SN 2020jfo
.jpg) Supernova 2020jfo is the bright star inside the Messier 61 galaxy. | |
| Type II (peculiar) | |
| Date | May 06, 2020 |
|---|---|
| Constellation | Virgo |
| Right ascension | 4h 28m 54.05s |
| Declination | 12° 21′ 50.480″ |
| Epoch | J2000 |
| Distance | 0.00502 redshift |
| Host | Messier 61 |
| Notable features | Detailed data on progenitor star in archives |
| Peak apparent magnitude | +16.01 |
SN 2020jfo was a type II supernova in the Messier 61 galaxy, first observed on 6 May 2020 with an apparent magnitude of 16.01. It was one of the first supernovae for which independent, multi-instrument data was collected before, during, and after the explosion.[1] Large astronomical surveys like Transiting Exoplanet Survey Satellite (TESS) and Pan-STARRS have played a role in data collection before and after these events.[2][3][4]
References
[edit]- ^ Dvorsky, George (October 22, 2021). "Observations of Exploding Star in 'Real Time' Deemed a Major Step Towards Predicting Supernovas". Gizmodo.
- ^ Sollerman, J. (July 30, 2021). "The Type II supernova SN 2020jfo in M 61, implications for progenitor system, and explosion dynamics". Astronomy & Astrophysics. 655: A105. arXiv:2107.14503. Bibcode:2021A&A...655A.105S. doi:10.1051/0004-6361/202141374. S2CID 239388865.
- ^ Vallely, P.J.; Kocanek, CS; Stanek, KZ; Fausnaugh, M; Shappee, BJ (February 2021). "High-cadence, early-time observations of core-collapse supernovae from the TESS prime mission". Monthly Notices of the Royal Astronomical Society. 500 (4): 5639–5656. arXiv:2010.06596. doi:10.1093/mnras/staa3675.
- ^ Jones, DO (2021). "The Young Supernova Experiment: Survey Goals, Overview, and Operations". The Astrophysical Journal. 908 (143): 143. arXiv:2010.09724. Bibcode:2021ApJ...908..143J. doi:10.3847/1538-4357/abd7f5. S2CID 224803297.
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