NGC 595
| Emission nebula | |
|---|---|
| H II region | |
 The center of NGC 595 as seen by the Hubble Space Telescope | |
| Observation data: J2000 epoch | |
| Right ascension | 01h 33m 33.53s[1] |
| Declination | 30° 41′ 29.8″[1] |
| Distance | 3,000,000[2] ly (920,000 pc) |
| Apparent dimensions (V) | 1′[2] |
| Constellation | Triangulum |
| Physical characteristics | |
| Radius | ~440 ly (135 pc) (estimated)[2] ly |
| Designations | IRAS F01307 3025[1] |
NGC 595 is a massive H II region in the Triangulum Galaxy. It was discovered by Heinrich Ludwig d'Arrest on October 1, 1864 and is one of the biggest H II regions in the Local Group.
References
[edit]- ^ a b c "NGC 595". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-02-19.
- ^ a b c "NGC 595: A Great Diffuse Nebula in M33". Retrieved 13 Jan 2013.
External links
[edit]
Media related to NGC 595 at Wikimedia Commons- NGC 595 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
| Location | Triangulum Galaxy → Triangulum subgroup →
Local Group → Local Sheet → Virgo Supercluster → Laniakea Supercluster → Local Hole → Observable universe → Universe Each arrow (→) may be read as "within" or "part of". |  |
|---|---|---|
| H II regions | ||
| Suspected satellite galaxies | ||
 | This nebula-related article is a stub. You can help Wikipedia by expanding it. |