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Buy Online Celestron nexstar 6se computerized telescope in Dubai
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Near the bus station in Pontoise (Cergy-Pontoise). The background color has been computerized (IPhoto, Picnik): it's not a so creepy one in reality!
Projet Complexité : ?
What is Cryptocurrency ?
A cryptographic money is a virtual or computerized cash that can be utilized to purchase labor and products; which infers there’s no actual coin or bill utilized and every one of the exchanges occur on the web. It utilized an online record with solid cryptography to guarantee that online exchanges are totally secure. Here, we have incorporated every one of the subtleties relating to digital currency like sorts, how it works, utilizes, how to purchase and store it.
Our 2010 Christmas lights in Round Rock, Texas consisted of 14,260 LED lights using around 1400 watts and less than 12 amps of electricity. The Christmas lights were synchronized to music by computer that people listen to on 106.9 FM. Lights were shown on CNN, GMA, KVUE, Fox New's O'Reilly Factor, and our local Fox station.
Heavily computerized, you can customized just about every menu to show you what you want to see. I'm guessing that with all this computerization it wouldn't be a bad idea to buy an extended warranty.
No cluttered chart hanging off your bed. All data is entered into networked laptops throughout the hospital.
Our 2010 Christmas lights in Round Rock, Texas consisted of 14,260 LED lights using around 1400 watts and less than 12 amps of electricity. The Christmas lights were synchronized to music by computer that people listen to on 106.9 FM. Lights were shown on CNN, GMA, KVUE, Fox New's O'Reilly Factor, and our local Fox station.
An old shelf slip from the original Marshall-Wythe Law Library faculty library collection, used up until computerization.
There are always a few houses with the computerized synchronized light show and a local FM transmitter. Crazy but cool.
Snowflake test with over 4000 lights.
Snowflakes are new for our 2011 ListenToOurLights Christmas show. The front of the house will be covered with snowflakes. After updating some of our 2010 songs and after sequencing a new song for 2011 it was time to see how it would look. So I hung the snowflakes on my garage shelves in the same configuration that I plan for the front of the house. Since the wreaths and 3' trees were easy to grab I threw those in too. The cactus is stored on the roof and I hooked him up as well.
The 2011 Snowflake test contains 4 Light-O-Rama controllers and over 4000 LED lights. There are 12 X 17.3" LED snowflakes (cool white and blue), 9 X 42" LED snowflakes (cool white), and 4 X DIY Snowflakes with 60 Blue LEDs each. The 3' trees each have 35 cool white LED lights.
Taken at the 1st Annual OLC (On Line Computerized) Cross Country Soaring Camp at Moriarty, New Mexico.
Would YOU like to know the computerized process of sales orders and creating a picklists in QuickBooks Enterprise advanced inventory? If yes, then you are here in right place. Through this write-up we are going to overview on this topic and provide you in-depth guide for creating picklists in QB enterprise advanced inventory. As creating a picklists is really essential for inventory monitoring,
I can only guess what strange service this business actually provides it's customers. Not sure that I really want to know or it would spoil the interesting alternatives that pop in my head when I think about it.
Date: 04/24/2004
Location: Scottsdale, AZ
goo.gl/XOI5Yw The Important benefit of Medical Coding Company is the reduction in operating cost, data accuracy, better accuracy, etc for healthcare and hospitals. Outsourcing medical coding jobs will considerably reduce the workload in your office.
21 October 2023, 01:56 UT; Stuart, Florida USA (Bortle 6).
Stellarvue SV80/9D doublet achromatic reflector at f/6. Mallincam DS10C camera, bin 1, exposure 30s, RGB24, gain maximum, stacked 170 frames, L-eNhance filter, no guiding, dark frames subtracted. Processed in DSS, GraXpertAI (saved without stretch), Siril, Registar, and PS.
Appearance: large, dim, face-on spiral galaxy, bright core, lumpy bulge, four loose spiral arms, boundary is diffuse and not well defined,some magenta knots in the arms, background is rich starfield. Unconfirmed: Globular cluster U62 (mag 15.5) in the Triangulum Galaxy appears to be captured at 05:00 from the galaxy core.
Clouds: clear
Transparency: 5
Seeing: Fair
From Wikipedia:
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.
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, and proximity to one another in the night sky. It also has an H II nucleus.
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, in some computerized telescope software, and in some public outreach websites. However, the SIMBAD Astronomical Database, a professional database, collates formal designations for astronomical objects and indicates that Pinwheel Galaxy refers to Messier 101, which several amateur astronomy resources including public outreach websites identify by that name, and that is within the bounds of Ursa Major.
Under exceptionally good viewing conditions with no light pollution, the Triangulum Galaxy can be seen by some people with the fully dark-adapted naked eye; to those viewers, it is the farthest permanent entity visible without magnification, being about half again as distant as Messier 31, the Andromeda Galaxy. It is a diffuse, or extended, object rather than a starlike point, even without magnification, because of its physical extent.
Its observability without optical aid ranges from being relatively easily seen by people using direct vision in deep rural locations under a dark, clear, transparent sky, to requiring use of averted vision by observers in locations beyond the suburbs in shallow rural areas under good viewing conditions. It is one of the reference objects of the Bortle Dark-Sky Scale.
Crumey has shown that although the total apparent V-magnitude of M33 is 5.72, it has an effective visual magnitude of approximately 6.6, meaning that a precondition for visibility is that the observer can see stars at least as faint as that latter figure. This is fainter than many people are able to see, even at a very dark site.
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.
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. When William Herschel compiled his extensive catalog of nebulae, he was careful not to include most of the objects identified by Messier. However, M33 was an exception, and he cataloged this object on September 11, 1784, as H V-17.
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.
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), 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.
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.
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, 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. 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). The Triangulum Galaxy is around 750,000 light years from the Andromeda Galaxy.
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). The average of 102 distance estimates published since 1987 gives a distance modulus of 24.69, or .883 Mpc (2,878,000 light-years).
The Triangulum Galaxy is a source of H2O maser emission. 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).
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. A distance of less than 300 kiloparsecs between the two supports this hypothesis.
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. Pisces VII/Triangulum (Tri) III may be another satellite of Triangulum.
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.
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. 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. This is an isolated galaxy and there are no indications of recent mergers or interactions with other galaxies, and it lacks the dwarf spheroidals or tidal tails associated with the Milky Way.
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.
The nucleus of this galaxy is an H II region, 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. However, the nucleus does not appear to contain a supermassive black hole, as a best-fit value of zero mass and an upper limit of 1,500 M☉ is placed on the mass of a central black hole based on models and the Hubble Space Telescope (HST) data. This is significantly lower than the mass expected from the velocity dispersion of the nucleus and far below any mass predicted from the disk kinematics. This may suggest that supermassive black holes are associated only with galaxy bulges instead of with their disks. Assuming that the upper limit of the central black hole is correct, it would be rather an intermediate-mass black hole.
The inner part of the galaxy has two luminous spiral arms, along with multiple spurs that connect the inner to the outer spiral features. The main arms are designated IN (north) and IS (south).
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.
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.) 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.
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. 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.
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. 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. 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. Other prominent HII regions in Triangulum include IC 132, IC 133, and IK 53.
The northern main spiral arm contains four large HII regions, while the southern arm has greater concentrations of young, hot stars. 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. As of 2008, a total of 100 supernova remnants have been identified in the Triangulum Galaxy, 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. M33 being a local galaxy, the Central Bureau for Astronomical Telegrams (CBAT) tracks novae in it along with M31 and M81.
About 54 globular clusters have been identified in this galaxy, but the actual number may be 122 or more. 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.
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.
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.
As mentioned above, M33 is linked to M31 by several streams of neutral hydrogen and stars, which suggests that a past interaction between these two galaxies took place from 2 to 8 billion years ago, and a more violent encounter will occur 2.5 billion years in the future.
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; 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. 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).
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blog post: kvkhai-studio.blogspot.com/2011/10/perfect-pearl.html ... pencil on paper, digital enhancement, computerized text addition, original poem, (c) 2011
Today’s electronic sign boards almost seem like something out of yesterday’s science fiction or fantasy movies. You may have been attracted to one of these computerized advertising displays when you visited a local shopping mall, theater, park, or similar public place. These digital signs can display just about any type of media that can be displayed within a traditional web browser. This includes text, graphics, videos, and even feeds from popular social media networks.
The additional benefit of electronic signage over regular Internet advertising is that these signs can be placed in just the right location to catch consumers at a very late stage in the buyer’s journey. With touch screens or feeds from social media, they can even create an interactive experience for your target audience. Because of this, they can get designed for a great variety of solutions.
What are Digital Signs?
A digital sign board consist of a high-resolution display monitor, a computerized device that usually also has Internet access, and software to manage content. Because some of these electronic boards seem so high tech, they might also appear difficult to understand. Actually, they are quite simple. This software is called a content management system, or CMS.
The computerized device may be hooked to the monitor with something as simple as the type of HDMI cable that you can use to hook your own laptop up to your home TV. Of course, commercial electronic display equipment is usually much more robust than the kind of electronics and accessories that you buy to use in your house.
Why Are Businesses Turning to Electronic Signs?
Computerized signs offer many advantages when compare to both print and traditional Internet advertising. This is mostly because they have been demonstrated to do a good job of attracting attention. As a side benefit, they are very easy to maintain.
Why should you consider an electronic sign if you already advertise online? While many web users are starting to see ads on their searches, favorite websites, and social media pages as spam, they aren’t likely to regard electronic boards the same way when they find them in shopping malls, their favorite stores, or even outdoors. In fact, in one recent study, 63 percent of consumers said that digital signs attracted their attention. Most marketers know that their ads don’t usually perform that well.
Why chose an electronic board over a paper one? When compared to posters or cardboard signs, electronic signs win because they can display dynamic content that is very easy to change. In fact, all content can be managed from a remote location, so there is no need to travel to the sign to change it. Furthermore, the sign’s manager can control the display on thousands of these signs from the same console. Finally, you won’t be wasting paper because everything gets displayed online.
Are Electronic Signs Effective?
These dynamic and attention-getting electronic billboards are attracting attention away from other marketing channels. They can be used to provide information, advertise sales, and even entertain. Companies and other organizations are discovering hundreds of uses for dynamic signs, and you are bound to figure out some for yourself.
The post What is Digital Signage? The Complete Guide for Businesses appeared first on Work Best Electric.
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Students line up for the first computerized Drop/Add - and the computers failed. 1989 - Photo by Gary Jugert
There are always a few houses with the computerized synchronized light show and a local FM transmitter. Crazy but cool.
Congresswoman Berkley toured Nevada Health Center to celebrate National Health Centers Week. Here the staff demonstrates their computerized patient records system.
1992 and digging dough still. Computerized mixing at Burwood and Homebush and manual dough transfer at Fremantle. No wonder the place was closed. No doubt an orphan in the Arnott business. Image from Fremantle City Library.
Getting property documents throughout Sindh is now made more accessible. You can get the computerized copy of your land record from any district.
Just visit the nearest People Service Center with your CNIC.
#BOR #Sindh #SindhZameen #Computerized #Land #Record #District #property
reminds me of those mouse ear hats at Disneyland where the old lady uses that metal machine to embroider your name. Only now it's all computerized which makes me a little sad
3000*1600 (mm)
max speed 800mm/s
operation or adjustment on software console
input buffer area 32M
unlimitable repeat
material thickness thickest 3mm
various clothes&auxiliary material
configuration the first three tools
pens,vibration knife,rotating
vacuum 5.5KW
Control circuit and driver numerical servo motor or step motor
data form HPGL
voltage 220V±10% 50Hz 380V±10% 50Hz
data port PCI port
data transmission speed 100MB/S
control operation PC software console
it can be adjusted on software console or keyboard
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