Emuhead
06-03-2022, 01:30 PM
NGC 3293 in the center of the image, is known as the Gem Cluster, and its an open cluster of young stars in the Carina constellation.
The brightest stars are blue supergiants and theres also a pulsating red supergiant, named V361 Carinae.
This region would have been a starless cloud of gas and dust about ten million years ago, and then star formation began.
NGC 3324 in the lower left of the image is an open cluster located 7,560 ly from Earth.
The intense ultraviolet radiation from several of NGC 3324's hot young stars causes the gas cloud to glow with rich colours, and combined with the stars stellar winds has blown open a hollow in the surrounding gas and dust.
It is closely associated with the emission nebula IC 2599, and the two are often confused as a single object which has been nicknamed the "Gabriela Mistral Nebula". This is due to its resemblance to the side profile of Chilean poet, who received the Nobel Prize for literature in 1945.
Taken 26.02.2022 from Bortle 6 skies, Melbourne, Victoria.
Quattro 10", EQ6R Pro, ASI2600MM Pro, 3nm Astrodon & RGB Astrodon filters, ASIAir Pro. 5 hours of integration (Ha, Oiii, RGB stars) combined in HaGO palette, and 6 hours of integration (same but including an hour of Sii) in the alternate palette.
It was a humid night so and dew formed on my primary mirror fairly early which I wasnt prepared for (any suggestions there would be very welcome) and so the nights data capture was cut short. Having said that I'm happy with the results.
Hope you like them!
Astrobin link here for HaGO version (https://www.astrobin.com/srljex/), and here for alternate version (https://www.astrobin.com/wpddhn/) including Siii.
The brightest stars are blue supergiants and theres also a pulsating red supergiant, named V361 Carinae.
This region would have been a starless cloud of gas and dust about ten million years ago, and then star formation began.
NGC 3324 in the lower left of the image is an open cluster located 7,560 ly from Earth.
The intense ultraviolet radiation from several of NGC 3324's hot young stars causes the gas cloud to glow with rich colours, and combined with the stars stellar winds has blown open a hollow in the surrounding gas and dust.
It is closely associated with the emission nebula IC 2599, and the two are often confused as a single object which has been nicknamed the "Gabriela Mistral Nebula". This is due to its resemblance to the side profile of Chilean poet, who received the Nobel Prize for literature in 1945.
Taken 26.02.2022 from Bortle 6 skies, Melbourne, Victoria.
Quattro 10", EQ6R Pro, ASI2600MM Pro, 3nm Astrodon & RGB Astrodon filters, ASIAir Pro. 5 hours of integration (Ha, Oiii, RGB stars) combined in HaGO palette, and 6 hours of integration (same but including an hour of Sii) in the alternate palette.
It was a humid night so and dew formed on my primary mirror fairly early which I wasnt prepared for (any suggestions there would be very welcome) and so the nights data capture was cut short. Having said that I'm happy with the results.
Hope you like them!
Astrobin link here for HaGO version (https://www.astrobin.com/srljex/), and here for alternate version (https://www.astrobin.com/wpddhn/) including Siii.