NGC 4090

In this article, we will explore all aspects related to NGC 4090. From its origin to its impact on today's society, through its applications in different areas, NGC 4090 has become a topic of growing interest in recent years. Through a detailed and rigorous analysis, we will examine its evolution over time, as well as its relevance today. Additionally, we will address the opinions of experts in the field, who will offer their perspectives and reflections on NGC 4090. By comparing different points of view and evaluating empirical evidence, this article aims to provide a comprehensive and complete view of NGC 4090.

NGC 4090
SDSS image of NGC 4090
Observation data (J2000 epoch)
ConstellationComa Berenices
Right ascension12h 05m 27.9s[1]
Declination20° 18′ 32″[1]
Redshift0.024460[1]
Heliocentric radial velocity7333 km/s[1]
Distance340 Mly (104 Mpc)[1]
Group or clusterNGC 4065 Group
Apparent magnitude (V)14.85[1]
Characteristics
TypeSab[1]
Size~135,000 ly (41.4 kpc) (estimated)[1]
Apparent size (V)1.2 x 0.5[1]
Other designations
UGC 07077, PGC 038288, MCG +04-29-015[1]

NGC 4090 is a spiral galaxy located 340 million light-years away[2] in the constellation Coma Berenices.[3] The galaxy was discovered by astronomer Heinrich d'Arrest on May 2, 1864[4] and is a member of the NGC 4065 Group.[5][6][7][8]

NGC 4090 hosts an AGN.[9]

On April 5, 2018 a type Ia supernova designated as SN 2018aqh was discovered in NGC 4090.[10][11][12][13]

See also

References

  1. ^ a b c d e f g h i j "NASA/IPAC Extragalactic Database". Results for NGC 4090. Retrieved 2019-02-10.
  2. ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2019-02-10.
  3. ^ "Revised NGC Data for NGC 4090". spider.seds.org. Retrieved 2019-02-10.
  4. ^ "New General Catalog Objects: NGC 4050 - 4099". cseligman.com. Retrieved 2019-02-03.
  5. ^ 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.
  6. ^ 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.
  7. ^ 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. S2CID 73667751.
  8. ^ 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. S2CID 15714969.
  9. ^ "NGC 4090". sim-id. Retrieved 2019-02-10.
  10. ^ "List of supernovae sorted by host name". Bright Supernova - Archives. Retrieved 2019-02-10.
  11. ^ "Bright Supernovae - 2018". rochesterastronomy.org. Retrieved 2019-02-11.
  12. ^ "SN 2018aqh | Transient Name Server". wis-tns.weizmann.ac.il. Retrieved 2019-02-11.
  13. ^ "SN2018aqh - The Open Supernova Catalog". Archived from the original on 2016-09-17. Retrieved 2019-02-11.