N41 (nebula) explained
N41 |
Radius Ly: | ~50 |
Constellation: | Dorado |
Dist Ly: | ~160,000-170,000 |
Dec: | [1] |
Epoch: | J2000.0 |
Type: | emission |
N41 (also known as LMC N41, LHA 120-N 41) is an emission nebula in the north part of the Large Magellanic Cloud in the Dorado constellation.[2] Originally catalogued in Karl Henize's "Catalogue of H-alpha emission stars and nebulae in the Magellanic Clouds" of 1956, it is approximately 100 light-years wide and 160,000-170,000 light-years distant.[3]
Notes and References
- LHA 120-N 41. 2021-03-17.
- Davies. R. D.. Elliott. K. H.. Meaburn. J.. 1976. The nebular complexes of the Large and Small Magellanic Clouds. Memoirs of the Royal Astronomical Society. 81. 89. 1976MmRAS..81...89D. 0369-1829. 117858790.
- Henize. Karl G.. September 1956. Catalogues of Hα-emission Stars and Nebulae in the Magellanic Clouds. The Astrophysical Journal Supplement Series. en. 2. 315. 1956ApJS....2..315H. 10.1086/190025. 0067-0049. 122024157.