NGC 456
Emission nebula in the constellation Tucana
From Wikipedia, the free encyclopedia
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]
| 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 |
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]
