Submission: 2018 September
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Re: Submission: 2018 September
Hola a todos os dejo esta nebulosa, M 20, espero que os guste;
estos son los datos:
M 20
TOMAS:
R: 14 Light de 300 segundos, 14 Darks, 30 Flats y 40 Bias
G: 12 Light de 300 segundos, 12 Darks, 30 Flats y 40 Bias
B: 12 Light de 300 segundos, 12 Darks, 30 Flats y 40 Bias
L: 17 Light de 300 segundos, 17 Darks, 30 Flats y 40 Bias
TEMPERATURA: -10 GRADOS
TUBO: FSQ 106 ED
CCD: SBIG ST-8300M
MONTURA: CGEM
CCD guiar: QHY5 II
LUGAR: LAS INVIERNAS (GUADALAJARA)
saludos
jose
estos son los datos:
M 20
TOMAS:
R: 14 Light de 300 segundos, 14 Darks, 30 Flats y 40 Bias
G: 12 Light de 300 segundos, 12 Darks, 30 Flats y 40 Bias
B: 12 Light de 300 segundos, 12 Darks, 30 Flats y 40 Bias
L: 17 Light de 300 segundos, 17 Darks, 30 Flats y 40 Bias
TEMPERATURA: -10 GRADOS
TUBO: FSQ 106 ED
CCD: SBIG ST-8300M
MONTURA: CGEM
CCD guiar: QHY5 II
LUGAR: LAS INVIERNAS (GUADALAJARA)
saludos
jose
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Re: Submission: 2018 September
Dusty Mars Spin 2018
Mars Album on Vimeo:
https://vimeo.com/album/5390444
Created from a Mars map containing images taken in Namibia, Africa.
Locations:
IAS-Observatory, Gamsberg
Hakos Guest Farm
Guest Farm Kiripotib
July 12 to July 31 2018.
Instruments:
28" Newtonian (3120mm), Gamsberg
20" Keller-Cassegrain (4500 mm), Hakos
C11, Dr. Vehrenberg Sternwarte, Hakos
Meade 12" LX200, Hakos
Meade 10" LX200, Kiripotib
Filters: Baader 610nm, IR pass, RGB
Amplification: Baader FFC 4-5x
www.apollo-13.eu
sebastian@voltmer.de
Clear skies,
Sebastian
Mars Album on Vimeo:
https://vimeo.com/album/5390444
Created from a Mars map containing images taken in Namibia, Africa.
Locations:
IAS-Observatory, Gamsberg
Hakos Guest Farm
Guest Farm Kiripotib
July 12 to July 31 2018.
Instruments:
28" Newtonian (3120mm), Gamsberg
20" Keller-Cassegrain (4500 mm), Hakos
C11, Dr. Vehrenberg Sternwarte, Hakos
Meade 12" LX200, Hakos
Meade 10" LX200, Kiripotib
Filters: Baader 610nm, IR pass, RGB
Amplification: Baader FFC 4-5x
www.apollo-13.eu
sebastian@voltmer.de
Clear skies,
Sebastian
Re: Submission: 2018 September
M31, the Andromeda center, a LRGB picture
https://www.astrobin.com/users/nvcchr1/
Copyright: Niels V. Christensen
https://www.astrobin.com/users/nvcchr1/
Copyright: Niels V. Christensen
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Re: Submission: 2018 September
An Edge-On Spiral Galaxy in Coma Berenices
NGC 4565, sometimes referred to as the Needle Galaxy, is an edge-on galaxy in the constellation Coma Berenices. One can see the galaxy's yellowish central core, which is divided by obscuring dust lanes running the length of the equatorial plane. Total exposure was 10 hrs 20 min taken with a Takahashi CCA-250 f/5 astrograph and QSI683wsg CCD camera (Astrodon Gen2 filters) on a Paramount ME in Mayhill, NM on the nights of 8, 15, 16 May; 17, 18 June 2018 ( 21 x 1200 sec lights; 4 x 1200 sec R; 3 x 1200 sec G; 3 x 1200 sec B all @ -20 degrees C; 24 darks; 128 bias; 128 flats for each channel). Processed in PixInsight 1.8.5.1353 Ripley (x 64). An annotated image can be found on the Amateur Astronomers facebook page https://www.facebook.com/AmateurAstronomersGroup
Larger image: http://astronomersgroup.org/gallery/dis ... fullsize=1
NGC 4565, sometimes referred to as the Needle Galaxy, is an edge-on galaxy in the constellation Coma Berenices. One can see the galaxy's yellowish central core, which is divided by obscuring dust lanes running the length of the equatorial plane. Total exposure was 10 hrs 20 min taken with a Takahashi CCA-250 f/5 astrograph and QSI683wsg CCD camera (Astrodon Gen2 filters) on a Paramount ME in Mayhill, NM on the nights of 8, 15, 16 May; 17, 18 June 2018 ( 21 x 1200 sec lights; 4 x 1200 sec R; 3 x 1200 sec G; 3 x 1200 sec B all @ -20 degrees C; 24 darks; 128 bias; 128 flats for each channel). Processed in PixInsight 1.8.5.1353 Ripley (x 64). An annotated image can be found on the Amateur Astronomers facebook page https://www.facebook.com/AmateurAstronomersGroup
Larger image: http://astronomersgroup.org/gallery/dis ... fullsize=1
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- Location: San Diego, CA
- Contact:
Re: Submission: 2018 September
NGC 7217. KG Observatory.
NGC 7217 is an unbarred spiral galaxy 50 million light-years from Earth in the constellation of Pegasus. It is receding from us at approximately 952 kilometers per second.
It is an active galaxy with an active galactic nucleus (a compact region at the center of a galaxy that has a much higher than normal luminosity, probably caused by accretion of mass by a supermassive black hole at the center of its host galaxy).
NGC 7217’s main features are the presence of three optical ring-like zones of stars concentric to its bright nucleus. It has a tight, flocculent spiral structure with two spiral arms in the region of the outer ring. This suggests that NGC 7217’s central regions have suffered several starbursts. The outer ring is dominated by bright blue stars and is the location of most of the recent star formation in the galaxy. Although the galaxy is very gas poor for a spiral, this ring is also where we find the hydrogen gas to be concentrated. The galaxy is surrounded by an extensive, nearly circular luminous halo.
Other features this galaxy has are the presence of a number of stars rotating in the opposite direction around the galaxy’s center to most of them and two distinct stellar populations: one of intermediate age on its innermost regions and a younger, metal-poor on its outermost ones. An additional noteworthy feature is a symmetric ring of dust that surrounds the nucleus. Other dust lanes are seen mainly on the near side of the galaxy.
It has been suggested these features were caused by a merger with another galaxy and, in fact, computer simulations show that NGC 7217 could have been a large lenticular galaxy that merged with one or two smaller gas-rich ones, becoming the spiral galaxy we see today.
Imaging telescope or lens:Planewave CDK24
Imaging camera:FLI Proline 16803
Mount:Planewave L600
Guiding camera:Starlight Xpress Ultrastar
Focal reducer:None
Software:Planewave PWI4, Planewave PWI3, PixInsight 1.8, Maxim DL6, PHD Guiding 2, Neat Image V7, Photoshop CS3, Sequence Generator Pro
Filters:Astrodon 50mm R, Astrodon 50mm B, Astrodon 50 mm G, Astrodon 50mm L
Accessories:FLI CFW-5-7, Astrodon Monster MOAG, Hedrick Focuser, Planewave Delta-T, Planewave EFA
Resolution: 1448x1379
Dates: Sept. 4, 2018, Sept. 5, 2018, Sept. 6, 2018
Frames:
Astrodon 50 mm G: 24x300" -20C bin 1x1
Astrodon 50mm B: 24x300" -20C bin 1x1
Astrodon 50mm L: 27x300" -20C bin 1x1
Astrodon 50mm R: 24x300" -20C bin 1x1
Integration: 8.2 hours
Darks: ~20
Flats: ~80
Flat darks: ~80
Bias: ~20
Avg. Moon age: 24.72 days
Avg. Moon phase: 24.48%
Mean SQM: 21.50
Astrometry.net job: 2238974
RA center: 331.965 degrees
DEC center: 31.360 degrees
Pixel scale: 0.468 arcsec/pixel
Orientation: 179.240 degrees
Field radius: 0.130 degrees
Locations: KG Observatory, Julian, CA, United States
Data source: Backyard
NGC 7217 is an unbarred spiral galaxy 50 million light-years from Earth in the constellation of Pegasus. It is receding from us at approximately 952 kilometers per second.
It is an active galaxy with an active galactic nucleus (a compact region at the center of a galaxy that has a much higher than normal luminosity, probably caused by accretion of mass by a supermassive black hole at the center of its host galaxy).
NGC 7217’s main features are the presence of three optical ring-like zones of stars concentric to its bright nucleus. It has a tight, flocculent spiral structure with two spiral arms in the region of the outer ring. This suggests that NGC 7217’s central regions have suffered several starbursts. The outer ring is dominated by bright blue stars and is the location of most of the recent star formation in the galaxy. Although the galaxy is very gas poor for a spiral, this ring is also where we find the hydrogen gas to be concentrated. The galaxy is surrounded by an extensive, nearly circular luminous halo.
Other features this galaxy has are the presence of a number of stars rotating in the opposite direction around the galaxy’s center to most of them and two distinct stellar populations: one of intermediate age on its innermost regions and a younger, metal-poor on its outermost ones. An additional noteworthy feature is a symmetric ring of dust that surrounds the nucleus. Other dust lanes are seen mainly on the near side of the galaxy.
It has been suggested these features were caused by a merger with another galaxy and, in fact, computer simulations show that NGC 7217 could have been a large lenticular galaxy that merged with one or two smaller gas-rich ones, becoming the spiral galaxy we see today.
Imaging telescope or lens:Planewave CDK24
Imaging camera:FLI Proline 16803
Mount:Planewave L600
Guiding camera:Starlight Xpress Ultrastar
Focal reducer:None
Software:Planewave PWI4, Planewave PWI3, PixInsight 1.8, Maxim DL6, PHD Guiding 2, Neat Image V7, Photoshop CS3, Sequence Generator Pro
Filters:Astrodon 50mm R, Astrodon 50mm B, Astrodon 50 mm G, Astrodon 50mm L
Accessories:FLI CFW-5-7, Astrodon Monster MOAG, Hedrick Focuser, Planewave Delta-T, Planewave EFA
Resolution: 1448x1379
Dates: Sept. 4, 2018, Sept. 5, 2018, Sept. 6, 2018
Frames:
Astrodon 50 mm G: 24x300" -20C bin 1x1
Astrodon 50mm B: 24x300" -20C bin 1x1
Astrodon 50mm L: 27x300" -20C bin 1x1
Astrodon 50mm R: 24x300" -20C bin 1x1
Integration: 8.2 hours
Darks: ~20
Flats: ~80
Flat darks: ~80
Bias: ~20
Avg. Moon age: 24.72 days
Avg. Moon phase: 24.48%
Mean SQM: 21.50
Astrometry.net job: 2238974
RA center: 331.965 degrees
DEC center: 31.360 degrees
Pixel scale: 0.468 arcsec/pixel
Orientation: 179.240 degrees
Field radius: 0.130 degrees
Locations: KG Observatory, Julian, CA, United States
Data source: Backyard
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- Science Officer
- Posts: 483
- Joined: Thu Oct 12, 2017 6:04 pm
Re: Submission: 2018 September
TRIFID NEBULA
I present to you, one of my most important works, an extremely difficult nebula to process, and I have never been so cold to get an image as it was in Munhoz - MG - -Brazil
high resolution: https://www.astrobin.com/full/364170/0/
Located approximately 5,000 light-years away, in the constellation Sagittarius.
A star-forming region in the plane of our galaxy, the object is an unusual combination, illustrates three different types of astronomical nebulae:
1) Red emission nebulae dominated by the light of hydrogen atoms.
2) Blue reflection nebulae produced by dust reflecting starlight
3) Dark nebulae, apparent "gaps" in the emission nebula, which cause trifurcarda appearance.
Equipments:
Apo 150mm Esprit
Qhy 16200 mm
55 x 300 sec LRGB
Date: August 9, 10 and 11, 2018
Munhoz - MG - Brazil
Copyright: Ferrnando Oliveira de Menezes
I present to you, one of my most important works, an extremely difficult nebula to process, and I have never been so cold to get an image as it was in Munhoz - MG - -Brazil
high resolution: https://www.astrobin.com/full/364170/0/
Located approximately 5,000 light-years away, in the constellation Sagittarius.
A star-forming region in the plane of our galaxy, the object is an unusual combination, illustrates three different types of astronomical nebulae:
1) Red emission nebulae dominated by the light of hydrogen atoms.
2) Blue reflection nebulae produced by dust reflecting starlight
3) Dark nebulae, apparent "gaps" in the emission nebula, which cause trifurcarda appearance.
Equipments:
Apo 150mm Esprit
Qhy 16200 mm
55 x 300 sec LRGB
Date: August 9, 10 and 11, 2018
Munhoz - MG - Brazil
Copyright: Ferrnando Oliveira de Menezes
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- Science Officer
- Posts: 483
- Joined: Thu Oct 12, 2017 6:04 pm
Re: Submission: 2018 September
MOON 82.9%
https://www.astrobin.com/full/365341/0/
Processing and Capture:
Sharpcap, As3 !, Photoshop and Lightroom.
Equipments:
Esprit 150mm triplet
1600mc
Baader IR cut
August 30, 2018
Sao Paulo-SP- Brazil
Copyright: Fernando Oliveira de Menezes
https://www.astrobin.com/full/365341/0/
Processing and Capture:
Sharpcap, As3 !, Photoshop and Lightroom.
Equipments:
Esprit 150mm triplet
1600mc
Baader IR cut
August 30, 2018
Sao Paulo-SP- Brazil
Copyright: Fernando Oliveira de Menezes
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- Science Officer
- Posts: 483
- Joined: Thu Oct 12, 2017 6:04 pm
Re: Submission: 2018 September
HELIX NEBULA
HELIX NEBULA
Planetary nebulae are actually the remains of stars that once looked a lot like our sun. These stars spend most of their lives turning hydrogen into helium in massive runaway nuclear fusion reactions in their cores. In fact, this process of fusion provides all the light and heat that we get from our sun. Our sun will blossom into a planetary nebula when it dies in about five billion years.
Best details:
https://www.astrobin.com/full/364180/0/
Equipaments
Apo 150mm Esprit
Qhy 16200 mm
55 x 300 sec LRGB
Date: August 9, 10 and 11, 2018
Munhoz - MG - Brazil
Copyright: Fernando Oliveira de Menezes
HELIX NEBULA
Planetary nebulae are actually the remains of stars that once looked a lot like our sun. These stars spend most of their lives turning hydrogen into helium in massive runaway nuclear fusion reactions in their cores. In fact, this process of fusion provides all the light and heat that we get from our sun. Our sun will blossom into a planetary nebula when it dies in about five billion years.
Best details:
https://www.astrobin.com/full/364180/0/
Equipaments
Apo 150mm Esprit
Qhy 16200 mm
55 x 300 sec LRGB
Date: August 9, 10 and 11, 2018
Munhoz - MG - Brazil
Copyright: Fernando Oliveira de Menezes
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- Science Officer
- Posts: 483
- Joined: Thu Oct 12, 2017 6:04 pm
Re: Submission: 2018 September
HELIX NEBULA
Planetary nebulae are actually the remains of stars that once looked a lot like our sun. These stars spend most of their lives turning hydrogen into helium in massive runaway nuclear fusion reactions in their cores. In fact, this process of fusion provides all the light and heat that we get from our sun. Our sun will blossom into a planetary nebula when it dies in about five billion years.
Best details:
https://www.astrobin.com/full/364180/0/
Equipaments
Apo 150mm Esprit
Qhy 16200 mm
55 x 300 seg LRGB
Date: August 9, 10 and 11, 2018
Munhoz - MG - Brazil
Copyright: Fernando Oliveira de Menezes
Planetary nebulae are actually the remains of stars that once looked a lot like our sun. These stars spend most of their lives turning hydrogen into helium in massive runaway nuclear fusion reactions in their cores. In fact, this process of fusion provides all the light and heat that we get from our sun. Our sun will blossom into a planetary nebula when it dies in about five billion years.
Best details:
https://www.astrobin.com/full/364180/0/
Equipaments
Apo 150mm Esprit
Qhy 16200 mm
55 x 300 seg LRGB
Date: August 9, 10 and 11, 2018
Munhoz - MG - Brazil
Copyright: Fernando Oliveira de Menezes
Re: Submission: 2018 September
Cat's Eye Nebula
Copyright: Christopher Sullivan
Full resolution available here: https://www.astrobin.com/full/348611/
Full resolution available here: https://www.astrobin.com/full/348611/
Re: Submission: 2018 September
M76: Little Dumbbell Nebula
Copyright Christopher Sullivan
Full resolution available here:
https://www.astrobin.com/full/364189/
Full resolution available here:
https://www.astrobin.com/full/364189/
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- Science Officer
- Posts: 117
- Joined: Sat Feb 07, 2015 7:38 pm
Re: Submission: 2018 September
Comet 21P in Auriga by Transient Astronomer, on Flickr
Image Credit and Copyright, Terry Hancock, Tom Masterson, Grand Mesa Observatory www.grandmesaobservatory.com
Image Credit and Copyright, Terry Hancock, Tom Masterson, Grand Mesa Observatory www.grandmesaobservatory.com
Re: Submission: 2018 September
Have to comment on a few more pictures here...
Raul Villaverde, alcarreño, that's a great portrait of Andromeda. I like that smallish "dust ring" surrounded by a large, "soft" outer disk and halo composed mostly of old stars.
Delberson, that is a beautiful portrait of open cluster M23!
SUN SI, checkmates, I'm usually not so interested in pictures of the Moon and planets, but yours is fantastically striking!
SpookyAstro, that's a truly lovely picture of Comet 21P in Auriga! Look at all those well-known nebulas and clusters, and look at the brilliant color contrast between the comet and the stars, and look at that ginormous age-old "spaghettified" supernova remnant at lower right - Simeis 147, right?
Ann
Raul Villaverde, alcarreño, that's a great portrait of Andromeda. I like that smallish "dust ring" surrounded by a large, "soft" outer disk and halo composed mostly of old stars.
Delberson, that is a beautiful portrait of open cluster M23!
SUN SI, checkmates, I'm usually not so interested in pictures of the Moon and planets, but yours is fantastically striking!
SpookyAstro, that's a truly lovely picture of Comet 21P in Auriga! Look at all those well-known nebulas and clusters, and look at the brilliant color contrast between the comet and the stars, and look at that ginormous age-old "spaghettified" supernova remnant at lower right - Simeis 147, right?
Ann
Color Commentator
Re: Submission: 2018 September
M110 (DSLR)
Copyright: Paolo Demaria
Image captured during XXVII Saint Barthelemy Star Party (AO, Italy).
Telescope: Skywatcher Newton 200/1000 with Baader RCC
Mount: Skywatcher Eq6Pro
Camera: Canon Eos 450D modified Baader
33 x 600s @800 ISO + 30 x 30 s @800ISO.
Full resolution: https://s8.postimg.cc/8fnesj2dx/M110_FINAL.jpg
Best Regards,
Paolo Demaria, Cuneo, Italy
Copyright: Paolo Demaria
Image captured during XXVII Saint Barthelemy Star Party (AO, Italy).
Telescope: Skywatcher Newton 200/1000 with Baader RCC
Mount: Skywatcher Eq6Pro
Camera: Canon Eos 450D modified Baader
33 x 600s @800 ISO + 30 x 30 s @800ISO.
Full resolution: https://s8.postimg.cc/8fnesj2dx/M110_FINAL.jpg
Best Regards,
Paolo Demaria, Cuneo, Italy
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- Contact:
Re: Submission: 2018 September
Re: Submission: 2018 September
From Cygnus to Sagittarius
Copyright: Jon Talbot
Imaged from the extremely dark skies of Likely Calif in June, the splendor of the Milky Way was high overhead in this 4 panel mosaic taken with a Canon 6D and 35mm lens.
Higher resolution images available here: http://www.starscapeimaging.com/page227/index.html
Copyright: Jon Talbot
Imaged from the extremely dark skies of Likely Calif in June, the splendor of the Milky Way was high overhead in this 4 panel mosaic taken with a Canon 6D and 35mm lens.
Higher resolution images available here: http://www.starscapeimaging.com/page227/index.html