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A failed supernova is an astronomical event in time domain astronomy in which a star suddenly brightens as in the early stage of a supernova, but then does not increase to the massive flux of a supernova. They could be counted as a subcategory of supernova imposters. They have sometimes misleadingly been called unnovae.[1]


Overview


Failed supernovae are thought to create stellar black holes by the collapsing of a red supergiant star in the early stages of a supernova. When the star can no longer support itself, the core collapses completely, forming a stellar-mass black hole, and consuming the nascent supernova without having the massive explosion. For a distant observer, the red supergiant star will seem to wink out of existence with little or no flare-up. The observed instances of these disappearances seem to involve supergiant stars with masses above 17 solar masses.

Failed supernovae are one of several events that theoretically signal the advent of a black hole born from an extremely massive star, others including hypernovae and long-duration gamma-ray bursts.


Structure and process


Theoretically, a red supergiant star may be too massive to explode into a supernova, and collapse directly into being a black hole, without the bright flash. They would however generate a burst of gravitational waves. This process would occur in the higher mass red supergiants, explaining the absence of observed supernovae with such progenitors.[2][3][4]


List of failed supernovae candidates


Event Date Location Notes
NGC3021-CANDIDATE-1 NGC 3021
09h 50m 55.39s +33° 33′ 14.5″		 Disappearance of a 25-30 MSun F8 supergiant observed in archival HST data [2][5]
N6946-BH1 March 2009 NGC 6946
20h 35m 27.56s +60° 08′ 08.2″		 Disappearance of an 18-25 MSun red supergiant [2][6][4]

References


  1. Woosley, S. E.; Heger, Alexander (2012). "Long Gamma-Ray Transients from Collapsars". The Astrophysical Journal. 752 (1): 32. arXiv:1110.3842. Bibcode:2012ApJ...752...32W. doi:10.1088/0004-637X/752/1/32. S2CID 119240065.
  2. Lee Billings (November 2015). "Gone Without A Bang". Scientific American. 313 (5): 26–27. Bibcode:2015SciAm.313e..26B. doi:10.1038/scientificamerican1115-26b. PMID 26638393.
  3. Jon Voisey (2 April 2011). "Finding the Failed Supernovae". Universe Today.
  4. Eugene Myers (27 September 2016). "This star was so massive it ate itself before it could go supernova". Astronomy Magazine.
  5. Reynolds, Thomas M.; Fraser, Morgan; Gilmore, Gerard (21 July 2015). "Gone without a bang: An archival HST survey for disappearing massive stars". Monthly Notices of the Royal Astronomical Society (published November 2015). 453 (3): 2885–2900. arXiv:1507.05823. Bibcode:2015MNRAS.453.2885R. doi:10.1093/mnras/stv1809. S2CID 119116538.
  6. Gerke, J. R.; Kochanek, C. S.; Stanek, K. Z. (6 November 2014). "The Search for Failed Supernovae with The Large Binocular Telescope: First Candidates". Monthly Notices of the Royal Astronomical Society (published July 2015). 450 (3): 3289–3305. arXiv:1411.1761. Bibcode:2015MNRAS.450.3289G. doi:10.1093/mnras/stv776. S2CID 119212331.



На других языках

- [en] Failed supernova

[ru] Неудавшаяся сверхновая

Неудавшаяся сверхновая (несостоявшаяся сверхновая, англ. Failed supernova) — звезда, которая в конце своей жизни коллапсирует в чёрную дыру без вспышки сверхновой[1].


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