| NGC 213 | |
|---|---|
| SDSS image of NGC 213 | |
| Observation data (J2000 epoch) | |
| Constellation | Pisces |
| Right ascension | 00h 41m 09.9940s [1] |
| Declination | +16° 28′ 09.508″ [1] |
| Redshift | 0.018166 [1] |
| Distance | 245.7 ± 17.2 Mly (75.32 ± 5.28 Mpc) [1] |
| Apparent magnitude (V) | 14.23 [1] |
| Characteristics | |
| Type | SB(rs)a [1] |
| Apparent size (V) | 1.7' × 1.4' [1] |
| Other designations | |
| IRAS F00384+1611, 2MASX J00411000+1628101, UGC 436, MCG +03-02-023, PGC 2469, CGCG 457-026 [1] | |
NGC 213 is a barred spiral galaxy located in the constellation Pisces. It was discovered on October 14, 1784, by William Herschel. [2]
According to the SIMBAD database, NGC 213 is an Active Galaxy Nucleus Candidate, i.e. it has a compact region at the center of a galaxy that emits a significant amount of energy across the electromagnetic spectrum, with characteristics indicating that this luminosity is not produced by the stars. [3]
One supernova has been observed in NGC 213: