TrevorW
14-12-2023, 06:30 PM
N11 (also known as LMC N11, LHA 120-N 11) is the brightest emission nebula in the north-west part of the Large Magellanic Cloud in the Dorado constellation. The N11 complex is the second largest H II region of that galaxy, the largest being the Tarantula Nebula. It covers an area approximately 6 arc minutes across.It has an elliptical shape and consists of a large bubble, generally clear interstellar area, surrounded by nine large nebulae. It was named by Karl Henize in 1956.When close-up, the nebula has pink clouds of glowing gas which resembles candy floss.It has been well studied over the years and extends 1,000 light-years across.
Its particularly notable features include a huge cavity measuring 80 by 60 pc and a five million year old central cluster (NGC 1761). It is surrounded by several ionized clouds where young O stars are forming.Several massive stars are within it, including LH 9, LH 10, LH 13, LH 14. It includes a supernova remnant N11L. In the very centre of NGC 1761 is a bright multiple star HD 32228 which contains a rare blue Wolf-Rayet star, type WC5 or WC6, and an O-type bright giant.
66x3min subs stacked and processed in SIRIL / PS captured 13/12/2023 Bortle 5/6 skies clear slight wind
Its particularly notable features include a huge cavity measuring 80 by 60 pc and a five million year old central cluster (NGC 1761). It is surrounded by several ionized clouds where young O stars are forming.Several massive stars are within it, including LH 9, LH 10, LH 13, LH 14. It includes a supernova remnant N11L. In the very centre of NGC 1761 is a bright multiple star HD 32228 which contains a rare blue Wolf-Rayet star, type WC5 or WC6, and an O-type bright giant.
66x3min subs stacked and processed in SIRIL / PS captured 13/12/2023 Bortle 5/6 skies clear slight wind