NGC_7619

NGC 7619

NGC 7619

Galaxy in the constellation Pegasus


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 ...

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]

In 1970, a type Ia supernova was detected within NGC 7619; it was subsequently designated SN 1970J.[8]


References

  1. "NGC 7619". Simbad. Université de Strasbourg/CNRS. Retrieved 2021-02-10.
  2. Randall, S. W.; Jones, C.; Kraft, R.; Forman, W. R.; Sullivan, E. (April 2009). "Merging Cold Fronts In The Galaxy Pair NGC 7619 AND NGC 7626". The Astrophysical Journal. 696 (2): 1431–1440. arXiv:0811.1217. Bibcode:2009ApJ...696.1431R. doi:10.1088/0004-637X/696/2/1431. S2CID 14950971.
  3. Edson, J. B.; Zwicky, F. (1941). "Remarks on the Pegasus Cluster of Nebulae". Proceedings of the National Academy of Sciences. 27 (8): 366–369. Bibcode:1941PNAS...27..366E. doi:10.1073/pnas.27.8.366. PMC 1078341. PMID 16588471.
  4. Seligman, Courtney. "New General Catalogue objects: NGC 7600 - 7649". cseligman.com. Retrieved 2021-02-10.
  5. Hubble, E.P. (1929). "A Clue to the Structure of the Universe". Leaflet of the Astronomical Society of the Pacific. 1 (23): 93. Bibcode:1929ASPL....1...93H.
  • Media related to NGC 7619 at Wikimedia Commons



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