SN 1998bw

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SN 1998bw
SN 1998bw.jpg
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]


  1. ^ 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/9806299free to read. Bibcode:1999ApJ...516..788W. doi:10.1086/307131. 
  2. ^ "Gamma-Ray Supernova 1998bw". The Anglo-Australian Observatory. Retrieved 2006-10-20. 
  3. ^ 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. 
  4. ^ "A Strange Supernova with a Gamma-Ray Burst". European Southern Observatory. Retrieved 2015-11-14.