View allAll Photos Tagged G65
-*- Virtual Diva Couture
VDC Ops Dress FATPACK
Available at Mainstore maps.secondlife.com/secondlife/Oppenheim/170/229/4001 For Legacy, Legacy Perky and Maitreya, Lara Petite,Hourglass and Freya Bodies
-*- :studiOneiro: Portrait D BENTO set /poses/ HUD
► Exclusive for POSE Fair ► Set of 6 Bento poses, 20% OFF during the event ► March 7th - 28th ► Surl for event: maps.secondlife.com/secondlife/Brookhurst%20Cove/40/95/23
-*- .::Indulge::. 2021 I-Wagon G65 ONE
maps.secondlife.com/secondlife/Indulge%20North/180/65/2153
-*- JEWELERY== CHOP ZUEY==
Athene Noctua Set - TxChnge
maps.secondlife.com/secondlife/Chop%20Zuey/82/152/28
-*- DOUX - Cara hairstyle
maps.secondlife.com/secondlife/equal10/231/127/90
-*- place== at home
-*- CATWA CATYA
-*- MAITREYA MESH BODY
The supernova remnant G65.3+5.7 in Cygnus is a huge structure with a size of ca. 3.5° x 4.5°.. It shows niche structures mainly in OIII. The object was discovered and classified as a SNR by Gulf et al. in 1977. Before its main elements Sh2-91, Sh2-94 and Sh2-96 were already catalogued in the Sharpless catalogue as single independent structures..The image was shot with my vintage SMC Pentax-M 135/3.5 lens at f/5.6.
SMC Pentax-M 135/3.5 on ASI2600 mm-pro
25 x 600 s HA
29 x 600 s OIII
N13MS - Gulfstream G-650/G-VI - Air Kaitar
at Toronto Lester B. Pearson Airport (YYZ)
c/n 6036 - built in 2012
Obscure industrial spur trackage with light, aging jointed rail - there are probably thousands still in existence that feed into the branch lines and main lines of this country’s vast rail network. – This one winds back into the Henry G. Meigs Paving Asphalts and Emulsions Company on the east side of Portage, Wisconsin and that is the locomotive of Canadian Pacific switch job X-G65 easing back out light engine after delivering a half-dozen or so tank cars to the end of the “Meigs spur”. -- May 26th, 2016 ~~ A Jeff Hampton Photograph ©
I discovered the Hazy Pearl Nebula last summer in the northeastern part of the supernova remnant SNR G 65.3 +5.7. in the constellation Cygnus. It was recently registrated as a new Planetary Nebula Candidate with the name Maa 1 (PN-G: 066.8+05.5).
SH2-914 and Sh2-96 area part of the much bigger SNR G65.3+5.7 in the constellation Cygnus. The image is an HOO combination with RGB stars.
ASI2600mm-pro and TS Photoline 130/910 mm.
63 x 600s Ha
53 x 600x OIII
82 x 30 s R
82 x 30 s B
82 x 30 s B
I am fascinated with faint supernova remnants. This one is particularity dim. It lies at the head of Cygnus the swan, on the border of Vulpecula. Located approximately 3,200 light years away.
Supernova remnants (SNR) are formed when a large star ends its life in a supernova explosion. About 300 of these remnants are currently known in our galaxy. One of the most famous remnants, the Veil Nebula, also located in the constellation of Cygnus. Although this is the most famous one in this constellation, it’s not the only SNR.
SNR G65.3+5.7 was discovered by Gull et al. (1977) during an OIII survey of the Milky Way. Some parts of this SNR were already catalogued by Stewart Sharpless in his SH2 catalog as SH2-91, SH2-94 and SH2-96, but they were not recognized as being part of a bigger structure at that time. The idea that they could be part of a larger SNR was postulated by Sidney van den Bergh in 1960, but it took until 1977 for this to be confirmed.
Image captured over 4 nights; 2023-08-14, 15, 16 & 24
24 hours total integration
Ha subs 35 * 1,200 sec = 11 hours 40 min
OIII subs 34 * 1,200 sec = 11 hours 20 min
RGB = 1 hour
Imaging Equipment:
Askar ACL200 200mm
Rainbow Astro RST-135,
QHY268M camera
HO 3.0nm filters
As you can imagine, it was unspeakably awesome cruising through Beverly Hills with this thing and the G65. And yes, this is pretty grainy, but seeing as it's a Huayra I think we can get over that.
Vor passender Kulisse zeigt sich der Museumswagen 177 (Gotha-Gelenkwagen, Baujahr 1967, Typ G-65) am Rathaus der brandenburgischen Hauptstadt.
Ai'zhai bridge is a high-speed passage in Xiangxi Tujia and Miao Autonomous Prefecture of Hunan Province, China. It is located on the Dehang Grand Canyon. It is a part of the northwest highway of Jishou City and a key control project of Baotou Maoming Expressway (National Highway G65).
矮寨大桥（Ai'zhai Bridge），是中国湖南省湘西土家族苗族自治州境内的高速通道，位于德夯大峡谷之上，是吉首市西北部公路的构成部分，也是包头—茂名高速公路（国家高速G65）关键控制性工程。
One of the rolling shots from late June I never got to editing. Quite an experience, cruising through the streets of Beverly Hills with this Huayra and its accompanying G65 at 1:30 in the morning...
💥 AURORA Naomie
💥 .::Indulge::. 2021 I-Wagon G65 NITE II BOX
TP .::INDULGE::. 🚀🚀🚀 5 sek 🚀🚀🚀
💥 .collection Lucie & Paul
Site where the John Brown Shipyard stood, Clydebank
The O.R.P. Piorun played a crucial role during the Clydebank Blitz. On March 13, 1941, the Polish destroyer was docked at the John Brown Shipyard for repairs when Clydebank was subjected to a devastating Luftwaffe air raid1. The crew of the O.R.P. Piorun actively defended the town by firing upon enemy aircraft, helping to prevent further destruction and loss of life. Their valiant efforts were later commemorated with a plaque, in Solidarity Plaza, dedicated to the crew's bravery.
Additionally, this plaque was installed at the site where the John Brown Shipyard once stood, commemorating the shipyard's significant contributions and the historical events that took place there.
---
ORP Piorun was an N-class destroyer operated by the Polish Navy in World War II. The word piorun is Polish for "Thunderbolt". Ordered by the Royal Navy in 1939, the ship was laid down as HMS Nerissa before being loaned to the Poles in October 1940 while still under construction.
Lunette TS 86/464 Quadruplet APO astrographe
Réducteur Televue x0.80
Focale 371mm à F 4.3
Monture EQ6 Pro
Autoguidage Lunette Williams Optique WO66 366mm
Camera Starshoot Autoguider
Imageur ZWO ASI2600MM Pro
Roue à FiltreZWO 7*36MM
Filtre Baader L, R, V, B ,S2, Ha et O3
Sky Quality 19.95
Magnitude CLASS 5 Bortle
SGP SEQUENCE GENERATOR PRO, SIRIL et UWE ASTRO TOOLS
52 x 10 min en O3 et
60 x 10 min en Ha
18H40 d'expostion
Highlighted Items Showcased for The Warehouse Sale - Second Life Shopping Event - Aug 2022
- lock&tuft / sledge [fatpack]
- SAC Scorpion EVO III SMG v1.01 FULL
- [SAC] AUG A3 Poses(Wear Me!)
- [SAC] Steyr AUG A3 v1.06 Full Box(Wear Me!)
- THIS IS WRONG Bleak tattoo - FATPACK (ADD)
*************************************************************
-BROWS-
Volkstone Anton HD Brows / FATPACK - Available at TMD Event - September 5th
-HAIRBASE-
Volkstone Denver Hairbase / FATPACK - Available at mainstore
-SKIN-
Volkstone Kurt Skin FatPack - Lelutka Evo X - Available at mainstore
-GLASSES-
BONDI. Silverhand Glasses - Available at Tokyo Zero
-PANTS-
-ODIREN- Stephen Pants FATPACK - Available at Mainstore
-SHOES-
[ VERSOV ] MACCOV_moccasins_FATPACK_ - Available at TMD
-BACKDROP-
.PALETO.Backdrop:. U5 - Available at Equal 10
-VEHICLE-
.::Indulge::. 2021 I-Wagon G65 NITE II - Available at Mainstore
-EARINGS-
[VEX] Diamond Stud V2 - VEXIIN / Available at Mainstore
-SPONSORS-
THE WAREHOUSE SALE EVENT
BONDI
.PALETO.
VERSOV
VEXIIN
Volkstone
.::Indulge::. Motorsports
Have always went to places that were always photographed and I do not know why when this is on my doorstep.
Here is the continuation of my large summer-2018 project.
I had imaged this region for about 13 nights altogether between July and October 2018. You can call me crazy, using so many nights for just one object, in a region where clear nights are rare :) But I really wanted to see if I could catch this beautiful Supernova remnant, and I'm glad it succeeded :)
Recently Pixinsight was supplied with the new Starnet++ module, which you can use to completely separate the stars from the background. I used this software to enhance the very weak nebulosity and was astonished to see how much more could be drawn from the background compared to the processing I did last year. All other processing was performed using Astropixelprocessor and photoshop.
Supernova remnants (SNR) are formed when a large star ends its life in a supernova explosion. About 300 of these remnants are currently known in our galaxy. One of the most famous remnants, the Veil Nebula, is located in the constellation of Cygnus. Although this is the most famous one in this constellation, it’s not the only SNR. Cygnus contains several obscure SNR’s, among which SNR 65.3+5.7 (also known as SNR 65.2+5.7).
SNR G65.3+5.7 was discovered by Gull et al. (1977) during an OIII survey of the Milky Way. Some parts of this SNR were already catalogued by Stewart Sharpless in his SH2 catalog as SH2-91, SH2-94 and SH2-96, but they were not recognized as being part of a bigger structure at that time. The idea that they could be part of a larger SNR was postulated by Sidney van den Bergh in 1960, but it took until 1977 for this to be confirmed.
This is one of the larger SNR in the sky spanning a region of roughly 4.0x3.3 degrees. Mavromatakis et al. (2002) determined the age of the SNR to be 20.000-25.000 years and the distance about 2.600 – 3.200 lightyears. The shell has a diameter of roughly 230 lightyears! This SNR is a predominantly OIII shell with also some H-alpha signal.
This supernova shell is quite weak and there are hardly any high-resolution images of this region. In the internet maybe 5-10 deep images of this shell can be found and, in most cases, they don’t cover the entire shell or the resolution is quite low because it was done by using photo lenses at short focal lengths. That’s why I decided to see if I could try to image the entire shell using my equipment, a TMB92 refractor in combination with a QSI583ws ccd camera. Because of its large size I needed to make a 3x3 mosaic to cover the whole region.
As so many nights were already necessary to cover the region in OIII I didn’t succeed in grabbing the H-alpha data, but on the internet I found the MDWsurvey (mdwskysurvey.org) initiated by David Mittelman (†), Dennis di Cicco, and Sean Walker (MDW). This is a marvelous project with the goal to image the entire northern sky in H-alpha at a resolution of 3.17”/pixel. I contacted them and told them of my effort to grab imagery of this SNR and they were very kind to provide me with the H-alpha imagery of this region, so that the entire SNR could be brought into view in reasonable high resolution.
This bicolor image shows a combination of about 53h of OIII data (made by myself) and 20 hours of Ha-data (made by the MDW survey) in a single image. In this way the full span of the shell can be seen in all its glory.
Image info:
H-alpha (astrodon 3nm, mdwskysurvey.org):
Telescope: Astro-physics AP130mm starfire
Camera: Fli Proline 16803
5 frames of 12x1200s each
OIII (astrodon 3nm):
Telescope: TMB92SS
Camera: QSI583ws
9 frames, 158 x 1200s total
This is a higher resolution and completely reprocessed version of my previous image.
Here is the result of my large summer-2018 project. I have been imaging this region for about 13 nights altogether between July and October 2018. You can call me crazy, using so many nights for just one object, in a region where clear nights are rare :) But I really wanted to see if I could catch this beautiful Supernova remnant, and I'm glad it succeeded :)
Supernova remnants (SNR) are formed when a large star ends its life in a supernova explosion. About 300 of these remnants are currently known in our galaxy. One of the most famous remnants, the Veil Nebula, is located in the constellation of Cygnus. Although this is the most famous one in this constellation, it’s not the only SNR. Cygnus contains several obscure SNR’s, among which SNR 65.3+5.7 (also known as SNR 65.2+5.7).
SNR G65.3+5.7 was discovered by Gull et al. (1977) during an OIII survey of the Milky Way. Some parts of this SNR were already catalogued by Stewart Sharpless in his SH2 catalog as SH2-91, SH2-94 and SH2-96, but they were not recognized as being part of a bigger structure at that time. The idea that they could be part of a larger SNR was postulated by Sidney van den Bergh in 1960, but it took until 1977 for this to be confirmed.
This is one of the larger SNR in the sky spanning a region of roughly 4.0x3.3 degrees. Mavromatakis et al. (2002) determined the age of the SNR to be 20.000-25.000 years and the distance about 2.600 – 3.200 lightyears. The shell has a diameter of roughly 230 lightyears! This SNR is a predominantly OIII shell with also some H-alpha signal.
This supernova shell is quite weak and there are hardly any high-resolution images of this region. In the internet maybe 5-10 deep images of this shell can be found and, in most cases, they don’t cover the entire shell or the resolution is quite low because it was done by using photo lenses at short focal lengths. That’s why I decided to see if I could try to image the entire shell using my equipment, a TMB92 refractor in combination with a QSI583ws ccd camera. Because of its large size I needed to make a 3x3 mosaic to cover the whole region.
As so many nights were already necessary to cover the region in OIII I didn’t succeed in grabbing the H-alpha data, but on the internet I found the MDWsurvey (mdwskysurvey.org) initiated by David Mittelman (†), Dennis di Cicco, and Sean Walker (MDW). This is a marvelous project with the goal to image the entire northern sky in H-alpha at a resolution of 3.17”/pixel. I contacted them and told them of my effort to grab imagery of this SNR and they were very kind to provide me with the H-alpha imagery of this region, so that the entire SNR could be brought into view in reasonable high resolution.
This bicolor image shows a combination of about 53h of OIII data (made by myself) and 20 hours of Ha-data (made by the MDW survey) in a single image. In this way the full span of the shell can be seen in all its glory.
Image info:
H-alpha (astrodon 3nm, mdwskysurvey.org):
Telescope: Astro-physics AP130mm starfire
Camera: Fli Proline 16803
5 frames of 12x1200s each
OIII (astrodon 3nm):
Telescope: TMB92SS
Camera: QSI583ws
9 frames, 158 x 1200s total
I discovered the Hazy Pearl Nebula last summer in the northeastern part of the supernova remnant SNR G 65.3 +5.7. in the constellation Cygnus. It was recently registrated as a new Planetary Nebula Candidate with the name Maa 1 (PN-G: 066.8+05.5).
Here is the result of my large summer-2018 project. I have been imaging this region for about 13 nights altogether between July and October 2018. You can call me crazy, using so many nights for just one object, in a region where clear nights are rare :) But I really wanted to see if I could catch this beautiful Supernova remnant, and I'm glad it succeeded :)
Supernova remnants (SNR) are formed when a large star ends its life in a supernova explosion. About 300 of these remnants are currently known in our galaxy. One of the most famous remnants, the Veil Nebula, is located in the constellation of Cygnus. Although this is the most famous one in this constellation, it’s not the only SNR. Cygnus contains several obscure SNR’s, among which SNR 65.3+5.7 (also known as SNR 65.2+5.7).
SNR G65.3+5.7 was discovered by Gull et al. (1977) during an OIII survey of the Milky Way. Some parts of this SNR were already catalogued by Stewart Sharpless in his SH2 catalog as SH2-91, SH2-94 and SH2-96, but they were not recognized as being part of a bigger structure at that time. The idea that they could be part of a larger SNR was postulated by Sidney van den Bergh in 1960, but it took until 1977 for this to be confirmed.
This is one of the larger SNR in the sky spanning a region of roughly 4.0x3.3 degrees. Mavromatakis et al. (2002) determined the age of the SNR to be 20.000-25.000 years and the distance about 2.600 – 3.200 lightyears. The shell has a diameter of roughly 230 lightyears! This SNR is a predominantly OIII shell with also some H-alpha signal.
This supernova shell is quite weak and there are hardly any high-resolution images of this region. In the internet maybe 5-10 deep images of this shell can be found and, in most cases, they don’t cover the entire shell or the resolution is quite low because it was done by using photo lenses at short focal lengths. That’s why I decided to see if I could try to image the entire shell using my equipment, a TMB92 refractor in combination with a QSI583ws ccd camera. Because of its large size I needed to make a 3x3 mosaic to cover the whole region.
As so many nights were already necessary to cover the region in OIII I didn’t succeed in grabbing the H-alpha data, but on the internet I found the MDWsurvey (mdwskysurvey.org) initiated by David Mittelman (†), Dennis di Cicco, and Sean Walker (MDW). This is a marvelous project with the goal to image the entire northern sky in H-alpha at a resolution of 3.17”/pixel. I contacted them and told them of my effort to grab imagery of this SNR and they were very kind to provide me with the H-alpha imagery of this region, so that the entire SNR could be brought into view in reasonable high resolution.
This bicolor image shows a combination of about 53h of OIII data (made by myself) and 20 hours of Ha-data (made by the MDW survey) in a single image. In this way the full span of the shell can be seen in all its glory.
Image info:
H-alpha (astrodon 3nm, mdwskysurvey.org):
Telescope: Astro-physics AP130mm starfire
Camera: Fli Proline 16803
5 frames of 12x1200s each
OIII (astrodon 3nm):
Telescope: TMB92SS
Camera: QSI583ws
9 frames, 158 x 1200s total
——— STRUMENTAZIONE ———
Obiettivo: Samyang 135mm f2
Camera: Zwo Asi 294 mc color pro
Montatura: Skywatcher AZ-EQ5
Autoguida: Zwo mini guide con zwo asi 224mc
Filtro: Optolong L-extreme
Software d'acquisizione Sgpro
————— FOTO ————
temp 0 con dark, flat e darkflat
300s x 302scatti
—— ELABORAZIONE ——
Pixinsight
Photoshop
SNR G65.3+5.7 ,"The Little veil nebula" (SH2-91 SH2-94 SH2-96) en HOO dans la constellation du cygne.
une belle galère pour photographier ces voiles trés discrets.
130 poses de 300s et 87 poses de 600s avec filtre idas NBZ
asi 2600 mc pro
ioptron GEM28
asiair pro
askar FMA 230
ciel bortle 6/7
siril, pixinsight,photoshop.
I spotted this parked outside Estate Motors today in Goldens Bridge, New York. The sticker price on this thing was $234,000.00
I could enjoy imaging of the SNR with my old telescope and another duo-narrowband filter. STC Astro Duo-Narrowband filter has a bit wider 7-12nm bandwidth compared to Optolong L-ultimate filter 3nm, but result was not so much different. Both were nice. There looked to exist many dark filaments in the area.
Spectroscopic Observations of the Supernova Remnant Candidates 3 C 400.2 and S91 by Sabbadin F and D'Odorico S 1976:
adsabs.harvard.edu/full/1976A%26A....49..119S
The SNR was imaged with CCD first in 2002:
arxiv.org/abs/astro-ph/0204079v1
equipment: Takahashi FSQ-106ED, Reducer QE 0.73x, STC Astro Duo-Narrowband Filter, and Canon EOS R-SP4II, modified by Seo-san on Sky-Watcher CQ350 Pro Equatorial mount, autoguided at a star nearby with hiro-design off-axis guider, ZWO ASI 120MM-mini, and PHD2 Guiding
exposure: 13 times x 1,200 seconds, 4 x 240 sec, and 4 x 60 seconds at ISO 6,400 and f/3.6
site: 2,360m above sea level at lat. 35 20 13 North and long. 138 43 57 East in parking on southern slope of Mt.Fuji 富士山富士宮口五合目駐車場 Ambient temperature was around 1 degrees Celsius or 34 degrees Fahrenheit. Wind was mild, and SQML was up to 20.80. Seeing was bad, and guide error RMS was around 1".
This car looks sick in pictures, but in person.. Wow. It's incredible. To see it driving on my first day in LA was even more special, since most people just see it parked at the Beverly Wilshire.