NGC 7619

Galaxy in the constellation Pegasus From Wikipedia, the free encyclopedia

NGC 7619

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]

Quick Facts Observation data (J2000 epoch), Constellation ...
NGC 7619
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SDSS image of NGC 7619
Observation data (J2000 epoch)
ConstellationPegasus
Right ascension23h 17m 14.524s[1]
Declination+08° 12 22.63[1]
Redshift0.01324[1]
Heliocentric radial velocity3,944 km/s[1]
Apparent magnitude (B)12.7[1]
Characteristics
TypeE2[1]
Other designations
UGC 12523, MCG +01-59-052, PGC 71121[1]
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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]

References

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