Community hub
0 subscribers8 pages, 0 posts
Recent from talks
All channels
Be the first to start a discussion here.
Be the first to start a discussion here.
Be the first to start a discussion here.
Be the first to start a discussion here.
Contribute something
Welcome to the community hub built to collect knowledge and have discussions related to NGC 327.
Nothing was collected or created yet.
NGC 327
View on Wikipediafrom Wikipedia
| NGC 327 | |
|---|---|
 | |
| Observation data (J2000 epoch) | |
| Constellation | Cetus |
| Right ascension | 00h 57m 55.3s[1] |
| Declination | −05° 07′ 50″[1] |
| Redshift | 0.018239[1] |
| Heliocentric radial velocity | 5,468 km/s[1] |
| Apparent magnitude (V) | 14.5b[1] |
| Characteristics | |
| Type | SBbc[1] |
| Apparent size (V) | 1.6' × 0.7'[1] |
| Other designations | |
| MCG -01-03-047, 2MASX J00575536-0507495, 2MASXi J0057553-050749, IRAS F0053-0524, 6dF J0057554-050750, PGC 3462.[1] | |
NGC 327 is a spiral galaxy in the constellation Cetus. It was discovered on September 27, 1864 by Albert Marth. It is described by Dreyer as "faint, small, extended."[2] It is nearby galaxies NGC 329, NGC 325 and NGC 321.
One supernova has been observed in NGC 327: SN 2021aclv (type Ia, mag. 17.3).[3]
See also
[edit]References
[edit]- ^ a b c d e f g h "NASA/IPAC Extragalactic Database". Results for NGC 0327. Retrieved September 2, 2016.
- ^ "New General Catalog Objects: NGC 300 - 349". Cseligman. Retrieved October 30, 2016.
- ^ "SN 2021aclv". Transient Name Server. IAU. Retrieved September 4, 2024.
External links
[edit]
Media related to NGC 327 at Wikimedia Commons
 | This spiral galaxy article is a stub. You can help Wikipedia by expanding it. |