NGC 4098

NGC 4098 is an interacting[2] pair of spiral galaxies[2][3] located 330 million light-years away[3] in the constellation Coma Berenices.[4] NGC 4098 was discovered by astronomer William Herschel on April 26, 1785. It was then rediscovered by Hershel on December 27, 1786 was listed as NGC 4099.[5] NGC 4098 is a member of the NGC 4065 Group.[6][7][8][9][10]

NGC 4098
SDSS image of NGC 4098.
Observation data (J2000 epoch)
ConstellationComa Berenices
Right ascension 12h 06m 03.9s[1]
Declination20° 36′ 22″[1]
Redshift0.024337[1]
Helio radial velocity7296 km/s[1]
Distance330 Mly (101 Mpc)[1]
Group or clusterNGC 4065 Group
Apparent magnitude (V)14.5[1]
Characteristics
TypeS?[1]
Size~105,000 ly (32.3 kpc) (estimated)[1]
Apparent size (V)0.8 x 0.4[1]
Other designations
NGC 4099, UGC 07091, PGC 038365, MCG +04-29-023, VV 061[1]

Supernova

A supernova of an unknown type which was designated as PSN J12060084+2036183 was discovered in NGC 4098 on April 25, 2015.[11][12][13]

Nearby galaxies

NGC 4098 is interacting with the galaxy pair VV 62.[2]

gollark: Not how it works.
gollark: Lots of nodes might be *worse* because weird scaling issues could crop up.
gollark: So decentralized krist may actually be flakier.
gollark: Distributed systems are hard.
gollark: The NIST is the National Institute of Standards and Technology in America.

See also

References
  1. "NASA/IPAC Extragalactic Database". Results for NGC 4098. Retrieved 2019-02-14.
  2. Freeland, E.; Stilp, A.; Wilcots, E. (2009-07-01). "H I Observations of Five Groups of Galaxies". The Astronomical Journal. 138 (1): 295–304. arXiv:0905.3907. Bibcode:2009AJ....138..295F. doi:10.1088/0004-6256/138/1/295. ISSN 0004-6256.
  3. "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2019-02-14.
  4. "Revised NGC Data for NGC 4098". spider.seds.org. Retrieved 2019-02-14.
  5. "New General Catalog Objects: NGC 4050 - 4099". cseligman.com. Retrieved 2019-02-03.
  6. Gregory, S. A.; Thompson, L. A. (1978-06-01). "The Coma/A1367 supercluster and its environs". The Astrophysical Journal. 222: 784–799. Bibcode:1978ApJ...222..784G. doi:10.1086/156198. ISSN 0004-637X.
  7. Tifft, W. G.; Gregory, S. A. (1979-07-01). "Band theory applied to the Coma/A1367 supercluster". The Astrophysical Journal. 231: 23–27. Bibcode:1979ApJ...231...23T. doi:10.1086/157158. ISSN 0004-637X.
  8. Burns, Jack O.; Hanisch, Robert J.; White, Richard A.; Nelson, Eric R.; Morrisette, Kim A.; Moody, J. Ward (1987-09-01). "A VLA 20 CM survey of poor groups of galaxies". The Astronomical Journal. 94: 587–617. Bibcode:1987AJ.....94..587B. doi:10.1086/114494. ISSN 0004-6256.
  9. White, Richard A.; Bliton, Mark; Bhavsar, Suketu P.; Bornmann, Patricia; Burns, Jack O.; Ledlow, Michael J.; Loken, Christen (1999-11-01). "A Catalog of Nearby Poor Clusters of Galaxies". The Astronomical Journal. 118 (5): 2014–2037. arXiv:astro-ph/9907283. Bibcode:1999AJ....118.2014W. doi:10.1086/301103. ISSN 0004-6256.
  10. Freeland, E.; Stilp, A.; Wilcots, E. (2009-07-01). "HI Observations of Five Groups of Galaxies". The Astronomical Journal. 138 (1): 295–304. arXiv:0905.3907. Bibcode:2009AJ....138..295F. doi:10.1088/0004-6256/138/1/295. ISSN 0004-6256.
  11. "List of supernovae sorted by host name". Bright Supernova - Archives. Retrieved 2019-02-14.
  12. "Bright Supernovae - 2015". rochesterastronomy.org. Retrieved 2019-02-14.
  13. "PSN%20J12060084+2036183 - The Open Supernova Catalog". Retrieved 2019-02-14.


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