List_of_novae_in_the_Milky_Way_galaxy

List of novae in the Milky Way galaxy

List of novae in the Milky Way galaxy

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This is a partial list of novae in the Milky Way galaxy that have been discovered and recorded since 1891. Novae are stars that undergo dramatic explosions, but unlike supernovae, these do not result in the destruction of the original star. The likely rate of novae in the Milky Way is about 40 per year,[1] but of these only about 10 per year are discovered by observers as of the 2000s (decade).[2] This list attempts to include only the brighter or more notable novae.

The Central Bureau for Astronomical Telegrams (CBAT) maintains a more complete list of novae in the Milky Way since 1612.[2]

For a list of novae in individual years, see instead: novae in 2018, novae in 2019.

Nomenclature

Novae are initially designated via a "Nova [genitive form of constellation name] [year of discovery]" format, e.g. "Nova Cygni 1974" and "Nova Scorpii 2010". An official permanent name is usually soon assigned by the General Catalog of Variable Stars using the GCVS format for the naming of variable stars. When more than one nova is discovered in a constellation in one year, a numeric suffix is appended; hence "Nova Sagittarii 2011 #2", "Nova Sagitarii 2011 #3", etc.

Nova Eridani 2009 (apparent magnitude ~8.4) during a full moon
More information Year, Nova ...

See also

Notes

  1. A higher magnitude means a lower brightness. i.e. T Aurigae (+3.8) was a brighter nova than HR Lyrae (+6.5)

References

  1. Prialnik, Dina. "Novae", pp. 1846-56, in Paul Murdin, ed. Encyclopedia of Astronomy and Astrophysics. London: Institute of Physics Publishing Ltd and Nature Publishing Group, 2001. ISBN 1-56159-268-4
  2. Burnham, Robert (2013) [1977]. Burnham's Celestial Handbook, Volume Three: An Observer's Guide to the Universe Beyond the Solar System. New York, New York: Courier Dover Publications. pp. 1460–62. ISBN 978-0-486-31803-5.
  3. Bianchini, A.; Tappert, C.; Canterna, R.; Tamburini, F.; Osborne, H.; Cantrell, K. (2003). "RW Ursae Minoris (1956): An Evolving Postnova System". The Publications of the Astronomical Society of the Pacific. 115 (809): 811–18. Bibcode:2003PASP..115..811B. doi:10.1086/376434. S2CID 123571502.
  4. "Archived copy". Archived from the original on 2007-03-02. Retrieved 2010-03-05.{{cite web}}: CS1 maint: archived copy as title (link)
  5. "Light Curve Generator: AAVSO Data for Nova DEL 2013". American Association of Variable Star Observers. August 16, 2013. Archived from the original on August 20, 2013. Retrieved August 16, 2013.
  6. IAU Circ., 9266, 2 (2013). Edited by Green, D. W. E.
  7. CBET 4080 (March 20, 2015)
  8. Alan MacRobert Nova Sagittarii: What a Long, Strange Fade It’s Been Sky and Telescope April 29, 2015
  9. "The International Variable Star Index". aavso.org. AAVSO. Retrieved 12 January 2021.
  10. Scagell, Robin (April 30, 2018). "Nova in Perseus".
  11. Drake, Jeremy J.; Ness, Jan-Uwe; Page, Kim L.; Luna, G. J. M.; Beardmore, Andrew P.; Orio, Marina; Osborne, Julian P.; Mróz, Przemek; Starrfield, Sumner; Banerjee, Dipankar P. K.; Balman, Solen; Darnley, M. J.; Bhargava, Y.; Dewangan, G. C.; Singh, K. P. (December 2021). "The Remarkable Spin-down and Ultrafast Outflows of the Highly Pulsed Supersoft Source of Nova Herculis 2021". The Astrophysical Journal Letters. 922 (2): L42. arXiv:2110.14058. Bibcode:2021ApJ...922L..42D. doi:10.3847/2041-8213/ac34fd. S2CID 239998563.
  12. Munari, U.; Valisa, P.; Dallaporta, S.; Maitan, A. (December 2021). "High ionization conditions finally emerge as Nova Cas 2021 (V1405 Cas) ends the plateau and embraces a steady decline". The Astronomer's Telegram. 15093: 1. Bibcode:2021ATel15093....1M. Retrieved 11 June 2022.
  13. "V0415 Mus". The International Variable Star Index. AAVSO. Retrieved 16 July 2022.

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