Back NGC 4625 Arabic NGC 4625 (مجره) ARZ IC 3675 AST NGC 4625 Azerbaijani NGC 4625 Byelorussian NGC 4625 BS NGC 4625 CE NGC 4625 German NGC 4625 DIQ NGC 4625 Esperanto
| NGC 4625 | |
|---|---|
 | |
| Observation data (J2000 epoch) | |
| Constellation | Canes Venatici[1] |
| Right ascension | 12h 41m 52.7s[2] |
| Declination | +41° 16′ 26″[2] |
| Redshift | 609 ± 1 km/s[2] |
| Apparent magnitude (V) | 13.2g[2] |
| Characteristics | |
| Type | SAB(rs)m pec[2] |
| Apparent size (V) | 1.3′ × 1.2′[2] |
| Notable features | Asymmetric; Single spiral arm[3] |
| Other designations | |
| IC 3675,[2] UGC 7861,[2] PGC 42607[2] | |
Preview warning: Page using Template:Infobox galaxy with unknown parameter "image_size"
NGC 4625 is a distorted dwarf galaxy in the constellation Canes Venatici. The galaxy is formally classified as a Sm galaxy, which means that its structure vaguely resembles the structure of spiral galaxies. The galaxy is sometimes referred to as a Magellanic spiral because of its resemblance to the Large Magellanic Cloud's single-arm structure.
- ^ R. W. Sinnott, ed. (1988). The Complete New General Catalogue and Index Catalogue of Nebulae and Star Clusters by J. L. E. Dreyer. Sky Publishing Corporation and Cambridge University Press. ISBN 978-0-933346-51-2.
- ^ a b c d e f g h i "NASA/IPAC Extragalactic Database". Results for NGC 4625. Retrieved 2006-12-07.
- ^ Cite error: The named reference
carnegieatlaswas invoked but never defined (see the help page).