| 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 an H II region in the Triangulum Galaxy. It was discovered by Heinrich Ludwig d'Arrest on October 1, 1864.
References
- ^ 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
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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. |