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NGC 456
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| NGC 456 | |
|---|---|
A detailed view of NGC 456 with JWST NIRCam | |
| Observation data (J2000 epoch) | |
| Right ascension | 01h 13m 44.4s[1] |
| Declination | −73° 17′ 26″[1] |
| Apparent dimensions (V) | 3.3′ × 2.7′[1] |
| Physical characteristics | |
| Other designations | Kron 65, Lindsay 94, DEM-S 147, ESO 29-38, LHA 115-N 83.[1] |
| Associations | |
| Constellation | Tucana |
NGC 456 is a nebula with an open cluster located in the constellation Tucana.[2] It was discovered on August 1, 1826, by James Dunlop. It was described by Dreyer as "pretty faint, pretty large, irregularly round, mottled but not resolved, 1st of several."[3]
The nebula of NGC 456 is also known as LHA 115-N 83 and often referred as just N83.[1][4] N83 is located next to N84 (NGC 460) and together they form a molecular cloud complex. N83/N84 is an isolated star-forming region in the southeast part of the Small Magellanic Cloud. The region contains a possible supernova remnant.[5] The N83C region was studied with ALMA. The researchers found peaks associated with young stellar objects. The molecular gas is located at the edges of the HII region.[4]

See also
[edit]References
[edit]- ^ a b c d e "NGC 456". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 9 May 2017.
- ^ "NGC 456 – Astrodrudis". Retrieved 2020-06-14.
- ^ "New General Catalog Objects: NGC 450 - 499". Cseligman. Retrieved May 9, 2017.
- ^ a b Muraoka, Kazuyuki; Homma, Aya; Onishi, Toshikazu; Tokuda, Kazuki; Harada, Ryohei; Morioka, Yuuki; Zahorecz, Sarolta; Saigo, Kazuya; Kawamura, Akiko; Mizuno, Norikazu; Minamidani, Tetsuhiro; Muller, Erik; Fukui, Yasuo; Meixner, Margaret; Indebetouw, Remy (2017-07-26). "ALMA Observations of N83C in the Early Stage of Star Formation in the Small Magellanic Cloud". The Astrophysical Journal. 844 (2): 98. arXiv:1706.04871. Bibcode:2017ApJ...844...98M. doi:10.3847/1538-4357/aa7a0b. ISSN 0004-637X. Archived from the original on 2024-04-15.
- ^ Bolatto, Alberto D.; Leroy, Adam; Israel, Frank P.; Jackson, James M. (2003-09-20). "Unusual CO Line Ratios and Kinematics in the N83/N84 Region of the Small Magellanic Cloud". The Astrophysical Journal. 595 (1): 167–178. arXiv:astro-ph/0306144. Bibcode:2003ApJ...595..167B. doi:10.1086/377230. ISSN 0004-637X. Archived from the original on 2024-09-13.