2000/09/01 by J. P. U. Fynbo, J. U. Fynbo, S. T. Holland +11 · 1 citation
Physics and Astronomy · #Astrophysical Phenomena and Observations #Gamma-ray bursts and supernovae #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.1086/312942
published as Astrophys.J. 542 (2000) L89-L93 · 12 pages, 2 figures, AASTeX v5.02 accepted for publication in ApJ Letters
arxiv created 2000/09/01 · openalex publication_date 2000/10/20 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/31
We present Hubble Space Telescope Space Telescope Imaging Spectrograph observations of ESO 184-G82, the host galaxy of the gamma-ray burst GRB 980425 associated with the peculiar Type Ic supernova SN 1998bw. ESO 184-G82 is found to be an actively star-forming SBc subluminous galaxy. We detect an object consistent with being a point source within the astrometric uncertainty of 0 018 of the position of the supernova. The object is located inside a star-forming region. The object is ≳1 mag brighter than expected for the supernova based on a simple radioactive decay model. This implies either a significant flattening of the light curve or a contribution from an underlying star cluster.