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Triangulum Galaxy
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Triangulum Galaxy
VST snaps a very detailed view of the Triangulum Galaxy.jpg
Galaxy Messier 33 in Triangulum
Observation data (J2000 epoch)
Pronunciation/traɪˈæŋɡjʊləm/
ConstellationTriangulum
Right ascension01h 33m 50.02s[1]
Declination+30° 39′ 36.7″[1]
Redshift-0.000607 ± 0.000010[1]
Helio radial velocity-179 ± 3 km/s[2]
Galactocentric velocity-44 ± 6 km/s[2]
Distance (comoving)970 kpc (3.2 Mly)[3]
Apparent magnitude (V)5.72[1]
Characteristics
TypeSA(s)cd[2]
Mass5 × 1010[4] M☉
Number of stars40 billion (4×1010)[6]
Size18.74 kpc (61,120 ly)
(diameter; 25.0 mag/arcsec2 B-band isophote)[5][6]
Apparent size (V)70.8 × 41.7 moa[1]
Other designations
NGC 0598, MCG+05-04-069, UGC 1117, PGC 5818[2]
The Triangulum Galaxy is a spiral galaxy 2.73 million light-years (ly) from Earth in the constellation Triangulum. It is catalogued as Messier 33 or NGC (New General Catalogue) 598. With the D25 isophotal diameter of 18.74 kiloparsecs (61,100 light-years), the Triangulum Galaxy is the third-largest member of the Local Group of galaxies, behind the Andromeda Galaxy and the Milky Way. It is one of the most distant permanent objects that can be viewed with the naked eye.[7]
The galaxy is the smallest spiral galaxy in the Local Group (although the smaller Large and Small Magellanic Clouds may have been spirals before their encounters with the Milky Way), and is believed to be a satellite of the Andromeda Galaxy or on its rebound into the latter due to their interactions, velocities,[8] and proximity to one another in the night sky. It also has an H II nucleus.[9]
Contents
1Etymology
2Visibility
3Observation history
4Properties
4.1Location – distance – motion
4.2Structure
4.3Star formation
4.4Discrete features
4.5Relationship with the Andromeda Galaxy
4.6Planetary nebulae
5See also
6References
7Further reading
8External links
Etymology
The galaxy gets its name from the constellation Triangulum, where it can be spotted.
It is sometimes informally referred to as the "Pinwheel Galaxy" by some astronomy references,[10] in some computerized telescope software, and in some public outreach websites.[11] However, the SIMBAD Astronomical Database, a professional database, collates formal designations for astronomical objects and indicates that Pinwheel Galaxy refers to Messier 101,[12] which several amateur astronomy resources including public outreach websites identify by that name, and that is within the bounds of Ursa Major.[13][14]
Visibility
Under exceptionally good viewing conditions with no light pollution, the Triangulum Galaxy can be seen with the 20/20 vision naked eye;[15] to those viewers, it will sometimes be the farthest permanent entity visible without magnification.[16][17] Its light diffuses (spreads) across a little more than a pinprick of the unmagnified sky, the cause of which is its broadness – this astronomers term a diffuse, rather than compact, object.
Observers range from finding the galaxy easily visible by direct vision in a truly dark (and impliedly dry, cloud-free) sky to needing to use averted vision in rural or suburban skies with good viewing conditions.[15] It has been chosen as one of the critical sky marks of the Bortle Dark-Sky Scale,[18] supported by its relative invariability, reasonable northern declination, and brightness described.
Observation history
The Triangulum Galaxy was probably discovered by the Italian astronomer Giovanni Battista Hodierna before 1654. In his work De systemate orbis cometici; deque admirandis coeli caracteribus ("About the systematics of the cometary orbit, and about the admirable objects of the sky"), he listed it as a cloud-like nebulosity or obscuration and gave the cryptic description, "near the Triangle hinc inde". This is in reference to the constellation Triangulum as a pair of triangles. The magnitude of the object matches M33, so it is most likely a reference to the Triangulum Galaxy.[19]
The galaxy was independently discovered by Charles Messier on the night of August 25–26, 1764. It was published in his Catalog of Nebulae and Star Clusters (1771) as object number 33; hence the name M33.[20] William Herschel compiled his extensive catalog of nebulae, he was careful not to include most of the objects identified by Messier.[21] However, M33 was an exception, and he cataloged this object on September 11, 1784, as H V-17.[22]
Herschel also cataloged the Triangulum Galaxy's brightest and largest H II region (diffuse emission nebula containing ionized hydrogen) as H III.150 separately from the galaxy itself; the nebula eventually obtained NGC number 604. As seen from Earth, NGC 604 is located northeast of the galaxy's central core. It is one of the largest H II regions known, with a diameter of nearly 1500 light-years and a spectrum similar to that of the Orion Nebula. Herschel also noted three other smaller H II regions (NGC 588, 592, and 595).
It was among the first "spiral nebulae" identified as such by Lord Rosse in 1850. In 1922–23, John Charles Duncan and Max Wolf discovered variable stars in the nebulae. Edwin Hubble showed in 1926 that 35 of these stars were classical Cepheids, thereby allowing him to estimate their distances. The results were consistent with the concept of spiral nebulae being independent galactic systems of gas and dust, rather than just nebulae in the Milky Way.[23]
NGC 604 in the Triangulum Galaxy
NGC 604 in the Triangulum Galaxy
Composite of about 54 different pointings with Hubble's Advanced Camera for Surveys.[24]
Composite of about 54 different pointings with Hubble's Advanced Camera for Surveys.[24]
Properties
The Triangulum Galaxy is the third largest member of the Local Group of galaxies. It has a diameter measured through the D25 standard - the isophote where the surface brightness of the galaxy reaches 25 mag/arcsec2, to be about 18.74 kiloparsecs (61,100 light-years),[5] making it roughly 60% the size of the Milky Way. It may be a gravitationally bound companion of the Andromeda Galaxy. Triangulum may be home to 40 billion stars, compared to 400 billion for the Milky Way, and 1 trillion stars for Andromeda Galaxy.[6]
The disk of Triangulum has an estimated mass of (3–6) × 109 solar masses, while the gas component is about 3.2 × 109 solar masses. Thus, the combined mass of all baryonic matter in the galaxy may be 1010 solar masses. The contribution of the dark matter component out to a radius of 55×103 ly (17 kpc) is equivalent to about 5 × 1010 solar masses.[4]
Location – distance – motion
Triangulum (M33; lower left of center) and Andromeda Galaxy (M31; above center)
Estimates of the distance from the Milky Way to the Triangulum Galaxy range from 2,380×103 to 3,070×103 ly (730 to 940 kpc) (or 2.38 to 3.07 Mly), with most estimates since the year 2000 lying in the middle portion of this range,[25][26] making it slightly more distant than the Andromeda Galaxy (at 2,540,000 light-years). At least three techniques have been used to measure distances to M 33. Using the Cepheid variable method, an estimate of 2,770×103 ± 130×103 ly (849 ± 40 kpc) was achieved in 2004.[27][28] In the same year, the tip of the red-giant branch (TRGB) method was used to derive a distance estimate of 2,590×103 ± 80×103 ly (794 ± 25 kpc).[29] The Triangulum Galaxy is around 750,000 light years from the Andromeda Galaxy.[30]
In 2006, a group of astronomers announced the discovery of an eclipsing binary star in the Triangulum Galaxy. By studying the eclipses of the stars, astronomers were able to measure their sizes. Knowing the sizes and temperatures of the stars, they were able to measure the absolute magnitude of the stars. When the visual and absolute magnitudes are known, the distance to the star can be measured. The stars lie at the distance of 3,070×103 ± 240×103 ly (941 ± 74 kpc).[25] The average of 102 distance estimates published since 1987 gives a distance modulus of 24.69, or .883 Mpc (2,878,000 light-years).[31]
The Triangulum Galaxy is a source of H2O maser emission.[32] In 2005, using observations of two water masers on opposite sides of Triangulum via the VLBA, researchers were, for the first time, able to estimate the angular rotation and proper motion of Triangulum. A velocity of 190 ± 60 km/s relative to the Milky Way was computed, which means Triangulum is moving towards Andromeda Galaxy and suggesting it may be a satellite of the larger galaxy (depending on their relative distances and margins of error).[8]
In 2004, evidence was announced of a clumpy stream of hydrogen gas linking the Andromeda Galaxy with Triangulum, suggesting that the two may have tidally interacted in the past. This discovery was confirmed in 2011.[33] A distance of less than 300 kiloparsecs between the two supports this hypothesis.[34]
The Pisces Dwarf (LGS 3), one of the small Local Group member galaxies, is located 2,022×103 ly (620 kpc) from the Sun. It is 20° from the Andromeda Galaxy and 11° from Triangulum. As LGS 3 lies at a distance of 913×103 ly (280 kpc) from both galaxies, it could be a satellite galaxy of either Andromeda or Triangulum. LGS 3 has a core radius of 483 ly (148 pc) and 2.6 × 107 solar masses.[35]
Pisces VII/Triangulum (Tri) III may be another satellite of Triangulum.[36]
Structure
Infrared image of M33 taken with the Spitzer Space Telescope
Ultraviolet image of M33 by GALEX observatory
In the French astronomer Gérard de Vaucouleurs' revised Hubble Sandage (VRHS) system of galaxy morphological classification, the Triangulum Galaxy is classified as type SA(s)cd. The S prefix indicates that it is a disk-shaped galaxy with prominent arms of gas and dust that spiral out from the nucleus—what is commonly known as a spiral galaxy. The A is assigned when the galactic nucleus lacks a bar-shaped structure, in contrast to SB class barred spiral galaxies. American astronomer Allan Sandage's "(s)" notation is used when the spiral arms emerge directly from the nucleus or central bar, rather than from an inner ring as with an (r)-type galaxy. Finally, the cd suffix represents a stage along the spiral sequence that describes the openness of the arms. A rating of cd indicates relatively loosely wound arms.[37]
This galaxy has an inclination of 54° to the line of sight from Earth, allowing the structure to be examined without significant obstruction by gas and dust.[38][39] The disk of the Triangulum Galaxy appears warped out to a radius of about 8 kpc. There may be a halo surrounding the galaxy, but there is no bulge at the nucleus.[40] This is an isolated galaxy and there are no indications of recent mergers or interactions with other galaxies,[39] and it lacks the dwarf spheroidals or tidal tails associated with the Milky Way.[41]
Triangulum is classified as unbarred, but an analysis of the galaxy's shape shows what may be a weak bar-like structure about the galactic nucleus. The radial extent of this structure is about 0.8 kpc.[42]
The nucleus of this galaxy is an H II region,[32] and it contains an ultraluminous X-ray source with an emission of 1.2 × 1039 erg s−1, which is the most luminous source of X-rays in the Local Group of galaxies. This source is modulated by 20% over a 106-day cycle.[43] However, the nucleus does not appear to contain a supermassive black hole, as an upper limit of 3,000 solar masses is placed on the mass of a central black hole based upon the velocity of stars in the core region.[44]
The inner part of the galaxy has two luminous spiral arms, along with multiple spurs that connect the inner to the outer spiral features.[38][39] The main arms are designated IN (north) and IS (south).[45]
Star formation
NGC 604, a star-forming region in the Triangulum Galaxy, as imaged by the Hubble Space Telescope.
In the central 4′ region of this galaxy, atomic gas is being efficiently converted to molecular gas, resulting in a strong spectral emission of CO. This effect occurs as giant molecular clouds condense out of the surrounding interstellar medium. A similar process is taking place outside the central 4′, but at a less efficient pace. About 10% of the gas content in this galaxy is in the molecular form.[38][39]
Star formation is taking place at a rate that is strongly correlated with local gas density, and the rate per unit area is higher than in the neighboring Andromeda Galaxy. (The rate of star formation is about 3.4 Gyr−1 pc−2 in the Triangulum Galaxy, compared to 0.74 in Andromeda.[46]) The total integrated rate of star formation in the Triangulum Galaxy is about 0.45 ± 0.1 solar masses per year. It is uncertain whether this net rate is currently decreasing or remaining constant.[38][39]
Based on analysis of the chemical composition of this galaxy, it appears to be divided into two distinct components with differing histories. The inner disk within a radius of 30×103 ly (9 kpc) has a typical composition gradient that decreases linearly from the core. Beyond this radius, out to about 82×103 ly (25 kpc), the gradient is much flatter. This suggests a different star formation history between the inner disk and the outer disk and halo, and may be explained by a scenario of "inside-out" galaxy formation.[40] This occurs when gas is accumulated at large radii later in a galaxy's life space, while the gas at the core becomes exhausted. The result is a decrease in the average age of stars with increasing radius from the galaxy core.[47]
Discrete features
Using infrared observations from the Spitzer Space Telescope, a total of 515 discrete candidate sources of 24 μm emission within the Triangulum Galaxy have been catalogued as of 2007. The brightest sources lie within the central region of the galaxy and along the spiral arms.
Many of the emission sources are associated with H II regions of star formation.[48] The four brightest HII regions are designated NGC 588, NGC 592, NGC 595, and NGC 604. These regions are associated with molecular clouds containing (1.2–4) × 105 solar masses. The brightest of these regions, NGC 604, may have undergone a discrete outburst of star formation about three million years ago.[49] This nebula is the second most luminous HII region within the Local Group of galaxies, at (4.5 ± 1.5) × 107 times the luminosity of the Sun.[46] Other prominent HII regions in Triangulum include IC 132, IC 133, and IK 53.[45]
The northern main spiral arm contains four large HII regions, while the southern arm has greater concentrations of young, hot stars.[45] The estimated rate of supernova explosions in the Triangulum Galaxy is 0.06 Type Ia and 0.62 Type Ib/Type II per century. This is equivalent to a supernova explosion every 147 years, on average.[50] As of 2008, a total of 100 supernova remnants have been identified in the Triangulum Galaxy,[51] the majority of which lies in the southern half of the spiral galaxy. Similar asymmetries exist for H I and H II regions, plus highly luminous concentrations of massive, O type stars. The center of the distribution of these features is offset about two arc minutes to the southwest.[45] M33 being a local galaxy, the Central Bureau for Astronomical Telegrams (CBAT) tracks novae in it along with M31 and M81.[52]
About 54 globular clusters have been identified in this galaxy, but the actual number may be 122 or more.[41] The confirmed clusters may be several billion years younger than globular clusters in the Milky Way, and cluster formation appears to have increased during the past 100 million years. This increase is correlated with an inflow of gas into the center of the galaxy. The ultraviolet emission of massive stars in this galaxy matches the level of similar stars in the Large Magellanic Cloud.[53]
In 2007, a black hole about 15.7 times the mass of the Sun was detected in this galaxy using data from the Chandra X-ray Observatory. The black hole, named M33 X-7, orbits a companion star which it eclipses every 3.5 days. It is the largest stellar mass black hole known.[54][55]
Unlike the Milky Way and Andromeda galaxies, the Triangulum Galaxy does not appear to have a supermassive black hole at its center. This may be because the mass of a galaxy's central supermassive black hole correlates with the size of the galaxy's central bulge, and unlike the Milky Way and Andromeda, the Triangulum Galaxy is a pure disk galaxy with no bulge.[56]
Relationship with the Andromeda Galaxy
Triangulum on the collision paths of the Milky Way and Andromeda galaxies.
As mentioned above, M33 is linked to M31 by several streams of neutral hydrogen[57] and stars,[57] which suggests that a past interaction between these two galaxies took place from 2 to 8 billion years ago,[58][59] and a more violent encounter will occur 2.5 billion years in the future.[57]
The fate of M33 was uncertain in 2009 beyond seeming to be linked to its larger neighbor M31. Suggested scenarios include being torn apart and absorbed by the greater companion, fueling the latter with hydrogen to form new stars; eventually exhausting all of its gas, and thus the ability to form new stars;[60] or participating in the collision between the Milky Way and M31, likely ending up orbiting the merger product and fusing with it much later. Two other possibilities are a collision with the Milky Way before the Andromeda Galaxy arrives or an ejection out of the Local Group.[61] Astrometric data from Gaia appears in 2019 to rule out the possibility that M33 and M31 are in orbit. If correct, M33 is on its first infall proper into the Andromeda Galaxy (M31).[62]
Planetary nebulae
Planetary nebulae are not only important contributors to the chemical enrichment of galaxies, but provide valuable information on single and binary stellar evolution. In addition, these objects seem to always produce very bright planetary nebulae with consistent luminosities, regardless of the galaxy's mass, age, or metallicity. This feature is very useful as a standard candle for distance measurements.
Large systematic research on this topic has been done by Rebeca Galera-Rosillo and co-authors in 2018.[63] This work benefited from the use of the INT and WHT telescopes located at La Palma island. As a result of this study, three new planetary nebulae were discovered.
Newly discovered PNe (2018), Rebeca named the PNe after her closest family members.
GCM 1 (Ovejisaurio),01:34:48.86+31:05:14.8
GCM 2, (Cuchilla Andante)01:33:45.20+30:21:22.0
GCM 3, (Sewi)01:33:52.30+30:21:12.0
How to create a MySQL database from the command line
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How to create a MySQL database from the command line
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How to repair a crashed WordPress database table
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Country: WEST GERMANY
Operator: DB
Item: STEAM
Class or Maker: DB/01.10coal
Wheel Arrangement or Type: 4-6-2
Number: 01.1086
Place details: KASSEL shed
Additional notes: -
Original source material: Agfa 35mm slide
Photographer: Graham T.V. Stacey
Copyright: Photographer
Library locator reference: GTVS.0010
30937 Transport Photograph Database
1966JUN13GTVS004cs
AkkenCloud™ at Staffing World 2013 in Orlando showing their features of recruiting database software among other industry companies.
Harry Gordon MCMILLAN 3267
Farrier Staff Sergeant Major; Veterinary Lieutenant; acting Captain [for 6mths from 10 May 1904]
6th Contingent SAW and WW1
Died 25 June 1943 aged 76 years
5 yrs Marsden Mounted Rifles; 2 yrs 6th NZMR in South Africa; 1 yr Lieutenant South Africa.
South African War, 1899-1902
Decorations: Queens Medal [SA War]; NZ Long and Efficient Medal
Born Auckland, 17 July 1870 [other info in records states 1872 which was written in his own handwriting]
Occupation: Blacksmith; Wheelwright and Coachbuilder
Parents born in Caithness, Scotland.
His Cenotaph database record:
muse.aucklandmuseum.com/databases/Cenotaph/33772.detail?O...
His South African military records are available:
archway.archives.govt.nz/ViewFullItem.do?code=20521886&am...
Records include copy of Army orders from Lord Kitchener to Government House, New Zealand indicating change of Harry’s rank.
As of January 1901 at attestation he was 30 years and 3 months old; 5ft 9.5 inches; 10st 12lb with 36.5 inch chest.
Tendered resignation as territorial soldier on 20 May 1912 after 19 years 8 mths continuous service. Wanted to be appointed Vet. Surgeon to 3rd Regiment Auckland Mounted Rifle Volunteers on is resigning command of the Scottish Horse Mounted Rifle Volunteers, but was declined due to being considered not having the correct qualifications.
He was married with 2 boys by March 1912 and his chest was 40 inches and weight 13st 6lb. He was Captain of B Squadron 11th Regiment and was a farmer. He desired to be a Sergeant Major Instructor.
Letter written to the Group Commander at Milton 23 March 1915 by Harry.
“Sir, in reference to my recent application for transfer to Auckland District, I wish to state for your information the following facts, which explain briefly the circumstances of my case, and the reasons for my application.
On my appointment as a Drill Instructor in May 1912 at Auckland, I was ordered to report myself at Dunedin, from whence I was posted to Lawrence. In addition to having to pay the expense of bringing my wife and 2 children from Auckland to Dunedin which cost me about £20, I had the misfortune to lose all my personal effects (about £50), through the wreck of the Auxiliary Scow which was bringing them from Whangarei to Auckland.
Shortly after my arrival at Lawrence, I had to refurnish my house at a cost of close on £400, and then had the further misfortune to lose everything by fire within 3 day of placing the furniture in my home and before I had had time to have the same insured.
Some 10 or 12 months ago, I was transferred to Wyndham and was just beginning to recover from my previous misfortunes, when in January of this year, I received the most crushing blow of all – the death of my wife. The result has been that I have had to sell up my home once more and am at present in lodgings with my two boys aged 6 and 8 respectively. As I am frequently away from home in attendance at Camps and parades etc, it means that my boys, who are now at a tender and impressionable age, cannot receive the attention they require. I have no relatives whatever in the South Island, but have 2 sisters in Auckland, who would be delighted to take charge of the boys: but as a father, I am very anxious not to be separated from them.
I am not aware of any N.C.O. in Auckland desirous of exchanging stations with me, nor am I able in my present circumstances to pay the cost of transfer.
My chain of misfortune seems to have been an endless one, and, as the future welfare of my children is so much at issue I sincerely trust that you will give my application your most favourable consideration.”
The response back was that at the present juncture his transfer would not be in the best interest of the service and it was suggested the ‘ladies’ might join their brother at Wyndham.
Further documentation shows that the citizens of Lawrence helped him out and that the only piece of furniture saved was a sewing machine. There is a good scan of a newspaper article about the fire in his military records archway.archives.govt.nz/ViewFullItem.do?code=20524602&am... the article in part states “…it appears the fire started in the bedroom occupied by the Sergeant’s two little boys …a small lamp being left burning [turned down] on a chest of drawers at the farther side of the room. Mr McMillan who fortunately, was at home, rushed into the bedroom, seized the children and succeeded with great difficulty in rescuing them from certain death. He twice fell getting them out, being overcome with the smoke, but on the last occasion this occurred in the passage where a rush of fresh air revived him and he was able to rise and carry his boys to safety. He is rather severely burned about the head, but regards this lightly in comparison with the saving of the lives of his children which he was able to effect.”
Thomas DRILLING the Town Clerk of Lawrence was instructed by the Mayor of Lawrence to write and inform Captain HENDERSON the area officer for Milton of the tragic impact on Harry and his family.
3 children [cannot trace 1] under 16 yrs of age by the time he attested to be in WW1 in 1917 aged 45 and stated that July 1915 he had been examined for military service in Milton, Otago and was found fit. Papers also show that he married Marcella BRENNAN in Wellington on 17 March 1917 [with children Norman Finlayson born 9 Jan 1906 and William John Markham 16 August 1908]. Marcella was his second marriage as Historic BDM search shows he wed Clara Eleanor MACRAE registered 1906/1659. Clara’s death registration is 1915/2483 and she was born 13 Dec 1877. Marcella died and is registered 1966/29735. Son Norman’s death registered 1983/27551 and William’s is registered 1981/41486]
Board of Enquiry in to the injury suffered by Harry. “…on moving from the parade ground to the Drill Hall at 8.30am on the 11th inst the squad moved at a fast pace as far as the back of the Grand Stand and were halted. As we proceeded to the hall my foot twisted and a sudden pain struck me above the knee of the left leg. I did not take any notice of it at the time. I carried on with physical drill as usual in the hall, after that we doubled back to our quarters for the rifles. As we fell in again to return to the hall the pain irritated me a little, but I carried on bayonet fighting. I carried on all day but I felt stiff at lunch time. I felt very sore after dinner. I reported to the Sergt Major at the medical hut at 6.30pm who applied hot fomentations and liniment. I saw the Medical Officer at 7.45 on the 12th inst. I suffered severe pain during the night and in the morning on getting up. I never had any injury before.” [Finding was that swelling and tenderness on pressure above the left knee is of opinion that the injury consists of partial separation of muscular fibres with effusion of blood in to the tissues.
Transferred from Group 5 Wellington to 17th Regiment as Regimental Sergeant Major. with effect from 25 Aug 1920.
Resigned as Sergeant Major NZ permanent staff from defence on 14 June 1925 and had a slightly damning ‘confidential’ report on him done 1924 stating “lacks administrative ability” online here archway.archives.govt.nz/ViewFullItem.do?code=20524602&am... all rather sad as he was obviously good enough in their eyes to serve 25 years in the military. Earlier confidential reports were fine.
Country: PORTUGAL
Operator: CP
Item: STEAM
Class or Maker: CP/E131
Wheel Arrangement: 2-8-2T
Number: E132
Place details: ESPINHO Station
Additional notes: 1000mm
Original source material: Agfa 35mm slide
Photographer: Robert W Bridger
Copyright: Photographer
Library locator reference: RWBR.0034
30937 Transport Photograph Database
1973MAY20RWBR001cs
/open N3 database
/archive
/experimental weapons
/Zero Point Energy Manipulator
/password: *********
/opening...please wait...
----
This is the first actual use of turquoise energy.
It can use green energy, turquoise energy, or the newly-found dark green energy.
Simply used for lifting things, but can damage flesh very badly. It can rip off your fibers, vessels; and can break your bones. Not even counting the internal bleeding.
You'll need to hold from the foregrip and the grip on the back. It doesn't really require much muscle power, but when throwing and picking it up, it can shake off pretty badly. So, foregrip is a must.
It doesn't use energy canisters, so it must be charged manually. Recharging back from the empty requires approximiately 3 hours.
Can hold on for 4 hours, or 1440 lift-offs.
-----------
I wonder why did anybody not think about this...
And no, gravity gun from HL2 was NOT my inspiration point.
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Baruch the Scribe (folk-pop)
Bosque Brown (country/soul)
Boxcar Bandits (skunkgrass)
Caleb Ian Campbell (singer-songwriter/experimental folk)
Curvette (experimental/post-punk/Southern rock)
Danny Rush and the Designated Drivers (country/rock)
Dear Human (post-rock)
Deep Snapper (post-punk)
Delmore Pilcrow (rock/country)
Depths (metal)
Dim Locator (avant-garde/Americana)
Drew Phelps (jazz)
Dust Congress (chamber folk)
Eaton Lake Tonics (experimental/folk/rock)
Ella Minnow (blues/pop/rock)
Final Club (rock)
Fishboy (indie-pop)
Jeremy Buller (singer-songwriter)
Jessie Frye (singer-songwriter/pop/rock)
Kaboom (rock)
Kampfgrounds (garage rock)
Land Mammals (psychedelic)
Magnum Octopus (hard rock)
Manned Missiles (garage rock/pop)
MATAS (indie/rock/pop)
Midnite Society (bloghaus)
Novaak (alternative/electronica/pop)
Oh Lewis (powerpop/Indie/rock)
On After Dark (indie/rock/new wave)
Paper Robot (rock)
Peoplodian (pop/electronic)
Pinebox Serenade (folk/rock)
Record Hop (rock)
Roy Robertson (experimental/folk)
RTB2 (experimental/ folk/rock/soul)
Sans Soleil (experimental/rock)
Seryn (folk/rock)
Sextape (ghettotech)
Shiny Around the Edges (experimental/punk)
Spooky Folk (indie-pop/rock)
Sundress (pop/psychedelic)
Swedish Teens (punk)
The Demigs (indie rock/pop)
The Hope Trust (rock/pop/country)
The Jakeys (acoustic/celtic/grunge)
The Slow Burners (folk/rock/psychedelic/roots)
The Wee-Beasties (alternative/punk/rock)
Violent Squid (experimental)
Westboro Butchers (rockabilly/instrumental)
Western Giants (Americana)
Western Skies (Americana)
Young and Brave (pop)
Adventures in Magnetism (Ft. Worth -- post-rock)
Air Review (Irving -- rock)
Analog Rebellion (Arlington -- stadium lo-fi)
AnonymousCulture (Dallas -- electronica/hip hop)
Baring Teeth (Dallas -- metal)
Broadcast Sea (Dallas -- rock)
Clint Niosi (Ft. Worth -- experimental/folk)
Cocky Americans (Dallas -- garage rock)
Diamond Age (Dallas -- acousmatic)
El Cento (Dallas -- rock)
Ethereal & the Queer Show (Dallas -- avant garde/pop)
Fate Lions (Ft. Worth -- pop/rock)
Here Holy Spain (Dallas -- skate punk/indie/rock)
Hormones (Dallas -- post-punk)
HOYOTOHO (Dallas -- alternative/big beat/live electronics)
Les Amercain (Dallas -- rock)
Man Factory (Grand Prairie -- powerpop/indie/rock)
Museum Creatures (Dallas -- concrete/garage /hard house)
myopic (Dallas -- ambient)
Nicolas Altobelli (Dallas -- folk)
Saboteur (Dallas -- emo/rock)
Salim Nourallah (Dallas -- folk)
Skeleton Coast (Ft. Worth -- rock/emo)
Somebody's Darling (Dallas -- country/rock)
Summer Ames (Dallas -- singer-songwriter/pop)
The Angelus (Dallas -- gospel/gothic/soul)
The Beaten Sea (Dallas -- country/folk/gothic)
The Bizarro Kids (Dallas -- experimental/psychedelic/trrash)
The Boom Boom Box (Plano -- post punk/rock)
The Burning Hotels (Ft. Worth -- rock/new wave)
The Hanna Barbarians (Ft. Worth -- psychedelic/blues/rock)
The Lo-fi Chorus (Dallas -- Americana/electroacoustic)
The Naptime Shake (Dallas -- country/folk/indie)
The Orbans (Ft. Worth -- alternative/folk/rock)
Two Knights (Arlington -- indie/rock/minimalist)
Whiskey Folk Ramblers (Ft. Worth -- Americana/folk/rock)
4th & Inchez (F.N.I.) (Houston -- hip-hop)
Crown Imperial (Norman, OK -- rock)
Fresh Millions (Austin -- experimental/electronic/instrumental/rock)
Horse Thief (Oklahoma City, OK -- folk/psychedelic)
Hotel Hotel (Austin -- ambient/blues/shoegaze)
KB the Boo Bonic (Austin -- hip hop)
Little Lo (Austin -- folk)
Moon (Oklahoma City, OK -- indie-pop/rock)
OK Sweetheart (Tulsa, OK -- indie-pop)
Paul Benjaman Band (Tulsa, OK -- funk/rock/Western swing)
People on Vacation (Austin -- pop)
Quiet Company (Austin -- indie rock/powerpop)
Sanctus Bellum (Houston -- doom metal)
Sphynx (Austin -- indie-pop)
The League of Extraordinary Gz (Austin -- hip hop)
The Lonesome Heroes (Austin -- Americana/folk)
The Manichean (Houston -- experimental/progressive)
The Non (Oklahoma City, OK -- experimental/instrumental/rock)
The Panda Resistance (Tulsa, OK -- indie rock/instrumental)
The Sour Notes (Austin -- folk rock/psychedelic/roots)
The Virgin Wolves (Bowie -- indie rock/pop)
The Zest of Yore (Austin -- lo-fi rock)
Tiger Darrow (Austin -- pop/folk)
Zorch (Austin -- experimental/electronic/instrumental/rock)
Yes, you can build a PC case out of LEGO. Just make sure that you get everything grounded. Having lots of windows and light on the inside? That's just over the top.
Viitekood / Reference code: ERA.1298.1.474.94
Kirje andmebaasis FOTIS / Description in the database FOTIS: www.ra.ee/fotis/index.php?type=2&id=764215
How to set up web-based database management system with Adminer
If you would like to use this photo, be sure to place a proper attribution linking to xmodulo.com
Cheyava Falls is the tallest waterfall in Arizona - beating out Angel Falls, Seven Cataracts and Carr Falls. On the World Waterfall Database Cheyava also rates as the highest in Magnitude and Aesthetics in AZ. www.world-waterfalls.com/database.php?s=T&t=G&cat...
Cheyava cascades from the North Rim on the southern end of the Walhalla Plateau north of Honan Point. Often the Falls are merely a wet streak on the Canyon Wall. But in the Spring after a wet winter as the snow on the North Rim melts, Cheyava Falls become truly impressive - cascading 800 feet down the Redwall Limestone. The longest drop is about 400 feet, then it cascades another 400 feet through a brushy slope and into Clear Creek. Thick foliage keeps you from reaching the base of the falls. Seeing Cheyava Falls flowing strong is high on the list for avid Grand Canyon Hikers.
Ellsworth Kolb named the Falls. www.grandcanyonhistory.org/09.html "After the USGS river trip in the summer of 1923, Colonel Claude H. Birdseye suggested that Ellsworth give it a name, preferably of Indian origin. Ellsworth supposed the water flowed only intermittently, and he suggested Cheyava, a Hopi word meaning intermittent river, " [25]
Here is my Hike Description and TripLog from HikeArizona.com
Kampung Sungai Ular, Cherating, Pahang, Malaysia.
Eichhornia crassipes (Mart.) Solms. Pontederiaceae. CN: [Malay - Keladi bunting, Kameling telur, Bunga jamban], Lilac devil, Water hyacinth. Native to Northern South America (French Guiana, Guyana, Suriname, Venezuela, Brazil). Widely naturalized in tropics and subtropics. Ornamental, Soil improver (green manure). Plants perennial , typically free-floating. Vegetative stems condensed, except when branching. Flowering stems erect , bending over after flowering, to 25 cm, distal internode less than 4 cm. Sessile leaves in basal rosette. Very prolific growth and the dense mat-like floating vegetation contributed to clogged drains, waterways and rivers. Probably the most aggressive aquatic weed ever known in the tropics. Eradication of filariasis was also claimed hindered by this plant due to the ability of the Mansonia mosquito larvae to breathe via the spongy airy roots.
Note: Stilted roots of Pandanus tectorius in the foreground.
Synonym(s):
Pontederia crassipes Mart.
Eichhornia speciosa Kunth [Illegitimate]
Piaropus crassipes (Mart.) Raf.
Eichhornia cordifolia Gand. [Illegitimate]
Eichhornia crassicaulis Schltdl.
Eichhornia crassicaulis Schlecht.
Heteranthera formosa Miq.
Ref. & suggested reading:
FRIM Flora Database
Kamus Dewan Bahasa dan Pustaka, Malaysia
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The Oracle SQL Developer Data Modeler relational model is an intermediate model between the logical model and the physical models. It supports relational design decisions independent of the constraints of the target physical platform(s). The relational model displays views, tables, columns and their datatypes and all relationships. Diagrams can be formatted to highlight groups of tables. In this example the tables assigned to different schema are highlighted through colour differentiation.
Day 3 Working session
The database of the Relational Machine
Archival process , Intermediae, Madrid
Read about the process
Country: GREAT BRITAIN
Operator: BLUEBELL RAILWAY
Item: SIGNAL
Class or Maker: -
Wheel Arrangement or Type: -
Number: -
Place details: HORSTED KEYNES Station Signal Box
Additional notes: -
Original source material: Kodak 35mm slide
Photographer: Robert W Bridger
Copyright: Photographer
Library locator reference: RWBR0099
30937 Transport Photograph Database
1970FEB01RWBR001cs