SkyViking
19-03-2014, 10:42 PM
Hi All,
I felt it was time to once again explore some of the lesser travelled paths in our Southern skies:
Here is my latest image with the new 12.5" f/4 scope, showing cometary Globules CG 30, CG 31 and CG 38 in Puppis.
These globules are very faint and they did take a reasonable amount of exposure (16 hours) to rein in even with this fast scope.
Link to high resolution image (4.2MB) (http://www.rolfolsenastrophotography.com/Astrophotography/Nebulae/i-W2Npd4z/X3)
About the image:
Pictured against the sprawling star fields and dark clouds of the Southern constellation Puppis are some ghostly glowing structures known as cometary globules. They owe their existence to complex interactions between gas and dust and the intense ultraviolet radiation from young O type stars in their neighbourhood. And possibly also to supernova explosions in the distant past.
Passing shock waves and radiation pressure have interacted with density fluctuations in the interstellar medium, and caused the formation of condensations called Bok globules. The radiation is also ionizing Hydrogen gas in the area, visible as the faint pink glow, while slowly eroding away the condensed globules and blowing their contents out into long tails, similar to that of a comet.
Radio observations from ESO's La Silla observatory in Chile have shown that the gas in the globules has a temperature of some 5,000 to 14,000 Kelvin.
Within the dense globules new stars are being born and at least one of these is visible as a bright orange glow in the dense upper right globule CG 30. This is a Herbig-Haro object (HH120); the result of plasma jets ejected from young protostars which collide with the surrounding gas and dust and cause the glowing emission.
These delicate light-year wide structures are relatively short lived and will ultimately succumb to the emerging radiation pressure from the very stars born within them. Within a few hundred thousand years a splendid cluster of young bright stars will emerge and take their place.
This particular region in the southern constellation of Puppis is very rich. Surrounding the globules are faint dark clouds and countless stars in all colours. The beautiful little blue reflection nebula on the left is Bran 106 / vdB-Ha 5.
Image details:
Date: 31st January and 2nd, 3rd, 25th, 27th February and 1st, 4th, 5th, 6th March 2014
Exposure: LRGB: 675:105:95:85 mins, total 16 hours @ -25C
Telescope: Homebuilt 12.5" f/4 Serrurier Truss Newtonian
Camera: QSI 683wsg with Lodestar guider
Filters: Astrodon LRGB E-Series Gen 2
Taken from my observatory in Auckland, New Zealand
Comments and critique is most welcome.
Regards,
Rolf
I felt it was time to once again explore some of the lesser travelled paths in our Southern skies:
Here is my latest image with the new 12.5" f/4 scope, showing cometary Globules CG 30, CG 31 and CG 38 in Puppis.
These globules are very faint and they did take a reasonable amount of exposure (16 hours) to rein in even with this fast scope.
Link to high resolution image (4.2MB) (http://www.rolfolsenastrophotography.com/Astrophotography/Nebulae/i-W2Npd4z/X3)
About the image:
Pictured against the sprawling star fields and dark clouds of the Southern constellation Puppis are some ghostly glowing structures known as cometary globules. They owe their existence to complex interactions between gas and dust and the intense ultraviolet radiation from young O type stars in their neighbourhood. And possibly also to supernova explosions in the distant past.
Passing shock waves and radiation pressure have interacted with density fluctuations in the interstellar medium, and caused the formation of condensations called Bok globules. The radiation is also ionizing Hydrogen gas in the area, visible as the faint pink glow, while slowly eroding away the condensed globules and blowing their contents out into long tails, similar to that of a comet.
Radio observations from ESO's La Silla observatory in Chile have shown that the gas in the globules has a temperature of some 5,000 to 14,000 Kelvin.
Within the dense globules new stars are being born and at least one of these is visible as a bright orange glow in the dense upper right globule CG 30. This is a Herbig-Haro object (HH120); the result of plasma jets ejected from young protostars which collide with the surrounding gas and dust and cause the glowing emission.
These delicate light-year wide structures are relatively short lived and will ultimately succumb to the emerging radiation pressure from the very stars born within them. Within a few hundred thousand years a splendid cluster of young bright stars will emerge and take their place.
This particular region in the southern constellation of Puppis is very rich. Surrounding the globules are faint dark clouds and countless stars in all colours. The beautiful little blue reflection nebula on the left is Bran 106 / vdB-Ha 5.
Image details:
Date: 31st January and 2nd, 3rd, 25th, 27th February and 1st, 4th, 5th, 6th March 2014
Exposure: LRGB: 675:105:95:85 mins, total 16 hours @ -25C
Telescope: Homebuilt 12.5" f/4 Serrurier Truss Newtonian
Camera: QSI 683wsg with Lodestar guider
Filters: Astrodon LRGB E-Series Gen 2
Taken from my observatory in Auckland, New Zealand
Comments and critique is most welcome.
Regards,
Rolf