SN 1998bw
| SN 1998bw | |
|---|---|
 | |
| Observation data | |
| Supernova type | Type Ic |
| Remnant type | ? |
| Host galaxy | ESO 184-G82 |
| Constellation | Telescopium |
| Right ascension | 19h 35m 03.30s |
| Declination | −52° 50′ 45.9″ |
| Galactic coordinates | 344.99 -27.72 |
| Discovery date | 26 April 1998 |
| Physical characteristics | |
| Progenitor | ? |
| Progenitor type | ? |
| Colour (B-V) | ? |
| Notable features | ? |
SN 1998bw was a rare broad-lined Type Ic[1] gamma ray burst supernova detected on 26 April 1998 in the ESO 184-G82 spiral galaxy, which some astronomers believe may be an example of a collapsar.[2] The supernova has been linked to GRB 980425, which was detected on 25 April 1998, the first time a gamma-ray burst has been linked to a supernova.[3] The supernova is approximately 140 million light years away, very close for a gamma ray burst source.[4]
References
- ↑ Woosley, S. E.; Eastman, Ronald G.; Schmidt, Brian P. (1999). "Gamma-Ray Bursts and Type Ic Supernova SN 1998bw" (PDF). The Astrophysical Journal 516 (2): 788–796. arXiv:astro-ph/9806299. Bibcode:1999ApJ...516..788W. doi:10.1086/307131.
- ↑ "Gamma-Ray Supernova 1998bw". The Anglo-Australian Observatory. Retrieved 2006-10-20.
- ↑ Vreeswijk, P.; Tanvir, N.; Galama, T. (2000). "Gamma-Ray Burst Afterglows: Surprises from the Sky". The ING Newsletter 2: 5. Bibcode:2000INGN....2....5V. Retrieved 2014-08-27.
- ↑ "A Strange Supernova with a Gamma-Ray Burst". European Southern Observatory. Retrieved 2015-11-14.
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