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SN 2020fqv

From Wikipedia, the free encyclopedia
2020 supernova event in the NGC 4568 spiral galaxy collision
SN 2020fqv
Supernova SN 2020fqv in the Butterfly Galaxy NGC 4568
Event typeSN IIb
DateMarch 31, 2020
Right ascension12h 36m 33.260s[1]
Declination+11° 13′ 53.87″[1]
EpochJ2000
Galactic coordinatesNGC 4568
Redshift0.007522
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SN 2020fqv was atype II supernova which occurred in March 2020 in thespiral galaxyNGC 4568, approximately 60 millionlight years fromEarth. The explosion was detected by both theZwicky Transient Facility and theTransiting Exoplanet Survey Satellite. Observations were obtained by theHubble Space Telescope both years before and just 26 hours after it exploded, as well as many other instruments, providing the first holistic view of such an event.[2][3][4][5][6]

Light curves for SN 2020fqv in fourphotometric bands, adapted from Tinyanontet al. (2021)[6]

The progenitor star is modelled to be ared supergiant with a radius of800±100 R and a mass of15±3 M, fairly typical of type II supernova progenitors.[6]

References

[edit]
  1. ^ab"SN 2020fqv".Transient Name Server. IAU supernova working group. Retrieved2022-02-28.
  2. ^"The last days of a massive star before it went supernova".SYFY Official Site. 2021-10-28. Retrieved2021-11-01.
  3. ^Gough, Evan (2021-10-29)."Quick Action Let Hubble Watch the Earliest Stages of an Unfolding Supernova Detonation".Universe Today. Retrieved2021-11-01.
  4. ^"Astronomers Observe 'Rosetta Stone of Supernovae' | Sci-News.com".Breaking Science News | Sci-News.com. 2021-11-25. Retrieved2021-10-30.
  5. ^Howell, Elizabeth (2021-10-25)."Hubble telescope spots doomed star that is the 'Rosetta stone' of supernovas".Space.com. Retrieved2021-10-30.
  6. ^abcTinyanont, Samaporn; Ridden-Harper, R; Foley, R J; Morozova, V; Kilpatrick, C D; Dimitriadis, G; DeMarchi, L; Gagliano, A; Jacobson-Galán, W V; Messick, A; Pierel, J D R (2021-10-26)."Progenitor and close-in Circumstellar Medium of Type II Supernova 2020fqv from high-cadence photometry and ultra-rapid UV spectroscopy".Monthly Notices of the Royal Astronomical Society.512 (stab2887):2777–2797.arXiv:2110.10742.doi:10.1093/mnras/stab2887.ISSN 0035-8711.
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