NGC 367
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From Wikipedia, the free encyclopedia
Spiral galaxy in the constellation Cetus
| NGC 367 | |
|---|---|
Pan-STARRS image of NGC 367 | |
| Observation data (J2000 epoch) | |
| Constellation | Cetus |
| Right ascension | 01h 05m 48.887s[1] |
| Declination | −12° 07′ 42.33″[1] |
| Redshift | 0.025999[1] |
| Heliocentric radial velocity | 7,693 km/s[2] |
| Apparent magnitude (V) | 14.7[3] |
| Characteristics | |
| Type | Sa[3] |
| Apparent size (V) | 0.9′ × 0.5′[3] |
| Other designations | |
| PGC 3894 | |
NGC 367 is a spiral galaxy in the constellation of Cetus. It was discovered in 1886 by the astronomer Frank Muller.[3]
References
[edit]- 1 2 3 "NGC 367". Simbad. Retrieved 2016-11-26.
- ↑ "Results for Object NGC 0367". NASA/IPAC Extragalactic Database. Archived from the original on 2016-11-27. Retrieved 2016-11-26.
- 1 2 3 4 "New General Catalog Objects: NGC 350 - 399". Cseligman. Retrieved 2016-11-26.
This spiral galaxy article is a stub. You can help Wikipedia by adding missing information. |
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