NGC 4090

In today's world, NGC 4090 has become a topic of great relevance and interest to a wide spectrum of society. Both on a personal and professional level, NGC 4090 has sparked numerous debates and discussions about its implications and consequences. From its origins to the present day, NGC 4090 has made a significant impact on the way we perceive the world around us. Over the years, NGC 4090 has evolved and adapted to the changes and challenges of the environment, demonstrating its ability to remain relevant and current in a world in constant transformation. In this article, we will explore in detail the multiple aspects and dimensions of NGC 4090, analyzing its influence in different areas of life and its role in shaping the present and the future.

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.