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NGC 7619 is an elliptical galaxy located in the constellation Pegasus.[2] NGC 7619 and NGC 7626[3] are the dominant and brightest members of the Pegasus galaxy cluster.[4] Both of them were discovered by William Herschel on September 26, 1785.[5]
| NGC 7619 | |
|---|---|
 SDSS image of NGC 7619 | |
| Observation data (J2000 epoch) | |
| Constellation | Pegasus |
| Right ascension | 23h 17m 14.524s[1] |
| Declination | +08° 12′ 22.63″[1] |
| Redshift | 0.01324[1] |
| Heliocentric radial velocity | 3,944 km/s[1] |
| Apparent magnitude (B) | 12.7[1] |
| Characteristics | |
| Type | E2[1] |
| Other designations | |
| UGC 12523, MCG +01-59-052, PGC 71121[1] | |
The radial velocity of this galaxy was measured in 1929 and found to be double that of any galaxy observed at that time.[6] The measurement was consistent with the extrapolated value predicted by Edwin Hubble; a distance-velocity relation that would later become known as Hubble's law.[7]
One supernova has been observed in NGC 7619: SN 1970J (type Ia, mag. 14.5) was discovered by Leonida Rosino on 24 September 1970.[8][9]
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