Ring Nebula (NGC 6822)
From Wikipedia, the free encyclopedia
| Diffuse nebula | Lists of nebulae |
|---|---|
| Observation data (Epoch J2000.0) |
|
| Type | Emission |
| Right ascension | 19h 44m 36s |
| Declination | -14° 41′ 42″ |
| Distance | 1.63 million ly |
| Apparent magnitude (V) | ~14.5 |
| Apparent dimensions (V) | 53″ |
| Constellation | Sagittarius |
| Physical characteristics | |
| Radius | |
| Absolute magnitude (V) | |
| Notable features | massive H II region |
| Other designations | Hubble 1925 III; Hodge 4;
NGC 6822B; NGC 6822-2 |
| edit | |
The Ring Nebula in Barnard's Galaxy has the official designation of Hubble 1925 III as it was the third (Roman numeral 3) object recorded in Hubble's 1925 paper, N.G.C. 6822, A Remote Stellar System. It includes areas of bright H II emission. In Paul W. Hodge's 1977 paper it was designated Hodge 4.
Its appearance is very similar to the filamentary nebula found in the Large Magellanic Cloud (see Meaburn 1981). It most resembles the circular ring-like nebula N70 in the LMC.
[edit] External links
 |
This astronomy related article is a stub. You can help Wikipedia by expanding it. |
