NGC 4589
NGC 4589 imaged by the Hubble Space Telescope
Observation data (J2000 epoch)
ConstellationDraco
Right ascension12h 37m 25.0s[1]
Declination+74° 11 30[1]
Redshift0.006511[2]
Heliocentric radial velocity1946 km/s[2]
Distance73.0 Mly (22.39 Mpc)[1]
Characteristics
TypeE[2]
Apparent size (V)3.47 × 2.75[3]
Other designations
IRAS F12353+7428, UGC 7797, LEDA 42139[2]

NGC 4589 is an elliptical galaxy located in the Draco constellation.[4][5][6] It is at a distance of about 108 million light-years away from the Earth. It is known by its designations PGC 42139 or UGC 7797.[2]

In the center of NGC 4589 lies a supermassive black hole. The galaxy hosted a supernova called 2005cz. NGC 4589 was discovered by astronomer William Herschel on November 22, 1797.

See also

References

  1. 1 2 3 Tully, R. Brent; et al. (August 2016). "Cosmicflows-3". The Astronomical Journal. 152 (2): 21. arXiv:1605.01765. Bibcode:2016AJ....152...50T. doi:10.3847/0004-6256/152/2/50. S2CID 250737862. 50.
  2. 1 2 3 4 5 "NGC 4589". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-01-14.
  3. Paturel, G.; et al. (December 2003). "HYPERLEDA. I. Identification and designation of galaxies". Astronomy and Astrophysics. 412: 45–55. Bibcode:2003A&A...412...45P. doi:10.1051/0004-6361:20031411.
  4. "Compass and Scale Image of Galaxies NGC 2768 and NGC 4589". HubbleSite.org. HubbleSite. Retrieved 2020-08-07.
  5. Lee, M.; et al. (2018-12-04). "Star Clusters in the Elliptical Galaxy NGC 4589 Hosting a Calcium-rich SN Ib (SN 2005CZ)". Retrieved 2020-08-07.
  6. Kawabata, K. S.; et al. (2010-05-20). "A massive star origin for an unusual helium-rich supernova in an elliptical galaxy". Nature. 465 (7296): 326–328. arXiv:0906.2811. Bibcode:2010Natur.465..326K. doi:10.1038/nature09055. PMID 20485430. S2CID 205220629.


This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.