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Sunday, January 16, 2011

A supernova remnant, the "Veil Nebula" reprocessed




Since my processing technique gets better and weather doesn't give any support, I have reprocessed some older images. There is now star colors added and other processing is tweaked too.


Veil Nebula
Ra 20h 45m 38.0s Dec +30° 42′ 30″






Image is in HST-palette, (HST=Hubble Space Telescope)
from the emission of ionized elements, R=Sulfur, G=Hydrogen and B=Oxygen.
Star colors are mixed from the NB channels, Red=H-a, G=O-III and B= 85%O-III + 15%H-a.


This very large SN locates in constellation Cygnus, about 2000 light years away. Angular diameter is about three degrees, about six full Moons side by side. Veil Nebula is one of the brightest features in the X-ray sky,
optically it has lowish surface brightness.






Natural color composition from the emission of ionized elements, R=80%Hydrogen+20%Sulfur, G=100%Oxygen and B=85%Oxygen+15%Hydrogen to compensate otherwise missing H-beta emission. This composition is very close to a visual spectrum. 
Star colors are mixed from the NB channels, Red=H-a, G=O-III and B= 85%O-III + 15%H-a.






An older image from 2007 of Eastern part of the nebula, NGC 6995. Sky Watcher 80 ED with an UHC-s filter and QHY8. Exposure time about 4h.




Original versions from Autumn 2008, with technical details:

I have made an experimental movie about the structure of the nebula. It can be found here:







Friday, January 14, 2011

NGC 6888, the "Crescent Nebula" reprocessed




Since my processing technique gets better and weather doesn't give any support, I have reprocessed some older images. There is now star colors added and other processing is tweaked too.

NGC 6888
Ra 20h 12m 7s  Dec +38° 21.3′[

Image is in HST-palette, (HST=Hubble Space Telescope)
from the emission of ionized elements, R=Sulfur, G=Hydrogen and B=Oxygen.
Star colors are mixed from the NB channels, Red=H-a, G=O-III and B= 85%O-III + 15%H-a.

The Crescent Nebula, also known as NGC 6888, Caldwell 27 and Sharpless 105, is an emission nebula in constellation Cygnus, about 5000 light years distance. 
It is formed by the fast stellar wind from the Wolf-Rayet star, WR 136 (HD 192163), colliding to an slower moving wind ejected by the same star when it became a red giant, around 400.000 years ago.
The result of the collision is a glowing shock shell around the star. Apparen size of the shell is 18' x 12' and the real size is about 25 x 16 light years. 




Natural color composition from the emission of ionized elements, R=80%Hydrogen+20%Sulfur, G=100%Oxygen and B=85%Oxygen+15%Hydrogen to compensate otherwise missing H-beta emission. This composition is very close to a visual spectrum. 
Star colors are mixed from the NB channels, Red=H-a, G=O-III and B= 85%O-III + 15%H-a.


Original version, Autumn 2009, with technical details:





NGC 6888 as a stereo pair 3D







Parallel vision 3D




Cross vision 3D



Original 2D:




NOTE! This is a personal vision about forms and shapes, based on some known facts and an artistic impression.


NGC 6888 as an anaglyph Red/Cyan 3D






You'll need Red/Cyan Eyeglasses to be able to see this image right.
Note, if you have a Red and Blue filters, you can use them! Red goes to Left eye.




Original 2D:





NOTE! This is a personal vision about forms and shapes, based on some known facts and an artistic impression.