Hi All, here is another new image from the large pile of data I was fortunate enough to gather during Dec-Jan. This time just under 11 hours on Thor's Helmet. I did plan to take some more colour data but I haven't had the chance since, so I've just combined what I had
Link to large image (2.5MB)
Link to medium resolution image
There is so much going on in this area so I had to also made a slightly different and closer crop to highlight the helmet area itself:
The link is here (1.3MB)
This delicate emission nebula is located in the constellation of Canis Major at a distance of about 15,000 light years. The nebula is illuminated by a central star in its last stage of life. This is a massive so called Wolf-Rayet star which is shedding its outer layers of gas at an extremely high rate due to intense radiation pressure. Wolf-Rayet stars are thought to represent a brief stage of evolution near the end of life for giant super massive stars - the last unstable phase before the star explodes as a brilliant supernova.
In the case of Thor's Helmet a large expanding bubble has formed around the bright central star. Interaction with giant molecular clouds in the area have contributed to the overall intricate shape of the nebula and large bow shock structures radiate out from the bubble in several directions. The nebula is some 30 light years in diameter and the strong blue-green colour is due to OIII emission near the star.
This entire spectacle lies embedded in a dense star field consisting of thousands of coloured jewels each casting their own contrasting light onto this dramatic interstellar scenery.
Image details:
Date: 8th, 14th, 19th December 2012 and 5th, 6th, 9th January 2013
Exposure: LRGB: 530:44:33:33m, total 10hrs 40mins @ -28C
Telescope: 10" Serrurier Truss Newtonian f/5
Camera: QSI 683wsg with Lodestar guider
Filters: Astrodon LRGB E-Series Gen 2
Taken from my observatory in Auckland, New Zealand
Personally I'm very happy with the outcome, I think this is one of my best images to date. However it is a
highly photogenic nebula so maybe that's why
Comments and critique welcome as always.
Regards,
Rolf