List of novae
Comment: Duplicates the mentioned list (the VAST majority of the novae on this list are from the Milky Way) and List of novae in 2018/List of novae in 2019, which also list extragalactic novae. Perhaps consider a move discussion to make the existing article a broader list. ᴢxᴄᴠʙɴᴍ (ᴛ) 07:32, 30 August 2026 (UTC)

A nova is a transient astronomical event that causes the sudden appearance of a bright, apparently "new" star (hence the name "nova", Latin for "new"; the shortened form of "stella nova", Latin for "new star") that slowly fades over weeks or months. All observed novae involve white dwarfs in close binary systems, but causes of the dramatic appearance of a nova vary, depending on the circumstances of the two progenitor stars. The main sub-classes of novae are classical novae, recurrent novae (RNe), and dwarf novae. They are all considered to be cataclysmic variable stars.
List of novae
See also
References
- ↑ Álvarez-Hernández, A.; Torres, M A P.; Rodríguez-Gil, P.; Shahbaz, T.; Anupama, G. C.; Gazeas, K. D.; Pavana, M.; Raj, A.; Hakala, P.; Stone, G.; Gomez, S.; Jonker, P. G.; Ren, J-J; Cannizzaro, G.; Pastor-Marazuela, I.; Goff, W.; Corral-Santana, J. M.; Sabo, R. (2021). "The intermediate polar cataclysmic variable GK Persei 120 years after the nova explosion: A first dynamical mass study". Monthly Notices of the Royal Astronomical Society. 507 (4): 5805–5819. arXiv:2107.06932. doi:10.1093/mnras/stab2547.
- ↑ Johnson, Christopher B.; Schaefer, Bradley E.; Kroll, Peter; Henden, Arne A. (2013). "Nova Aquilae 1918 (V603 Aql) Faded by 0.44 mag/century from 1938-2013". The Astrophysical Journal. 780 (2): L25. arXiv:1310.6802. Bibcode:2014ApJ...780L..25J. doi:10.1088/2041-8205/780/2/L25. Unknown parameter
|s2cid=ignored (help) - ↑ Ashok, N. M.; Banerjee, D. P. K. (October 2003). "The enigmatic outburst of V445 Puppis – A possible helium nova?". Astronomy and Astrophysics. 409 (3): 1007–1015. arXiv:astro-ph/0307304. Bibcode:2003A&A...409.1007A. doi:10.1051/0004-6361:20031160. Unknown parameter
|s2cid=ignored (help) - ↑ Goranskij, V. P.; Barsukova, E. A.; Burenkov, A. N.; Valeev, A. F.; Zharova, A. V.; Kroll, P.; Metlova, N. V.; Shugarov, S. Yu. (2020). "Progenitor and Remnant of the Luminous Red Nova V838 Monocerotis". Astrophysical Bulletin. 75 (3): 325–349. Bibcode:2020AstBu..75..325G. doi:10.1134/S1990341320030049. Unknown parameter
|s2cid=ignored (help) - ↑ Zemko, P.; et al. (August 2016). "V4743 Sgr, a magnetic nova?". Monthly Notices of the Royal Astronomical Society. 460 (3): 2744–2751. arXiv:1606.00225. Bibcode:2016MNRAS.460.2744Z. doi:10.1093/mnras/stw1199.
- ↑ 6.0 6.1 "VSX : Detail for RS Oph". vsx.aavso.org. Retrieved 2026-08-28.
- ↑ "2018bwo | Transient Name Server". www.wis-tns.org. Retrieved 2026-08-28.
- ↑ "VSX : Detail for YZ Ret". vsx.aavso.org. Retrieved 2026-08-28.
- ↑ "VSX : Detail for V0415 Mus". vsx.aavso.org. Retrieved 2026-08-28.
- ↑ Seach, John; Pearce, Andrew; Yoshimoto, K.; Guido, E.; Rocchetto, M.; McNaught, R. H.; Amorim, A.; Aguiar, J. G. de S.; Souza, W.; Camargo Da Silva, L.; Kazarovets, E. (2025). "V572 Velorum = Nova Velorum 2025 = PNV J10251200-5331109". Central Bureau Electronic Telegrams (5574): 1. Bibcode:2025CBET.5574....1S.
- ↑ "VSX : Detail for V0572 Vel". vsx.aavso.org. Retrieved 2026-08-28.
- ↑ "2025abao | Transient Name Server". www.wis-tns.org. Retrieved 2026-08-28.
External links
- Transient Name Server (TNS)
- Nova through 2015 at IAU Central Bureau for Astronomical Telegrams (CBAT)
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