HST/STIS Imaging of the Host Galaxy of GRB980425/SN1998bw
| dc.creator | Fynbo, J. U. | |
| dc.creator | Holland, S. | |
| dc.creator | Andersen, M. I. | |
| dc.creator | Thomsen, B. | |
| dc.creator | Hjorth, J. | |
| dc.creator | Bjornsson, G. | |
| dc.creator | Jaunsen, A. O. | |
| dc.creator | Natarajan, P. | |
| dc.creator | Tanvir, N. | |
| dc.date | 2000-09-01 | |
| dc.date.accessioned | 2026-07-07T01:55:15Z | |
| dc.date.available | 2026-07-07T01:55:15Z | |
| dc.description | We present HST/STIS observations of ESO 184-G82, the host galaxy of the gamma-ray burst GRB 980425 associated with the peculiar Type Ic supernova SN1998bw. ESO 184-G82 is found to be an actively star forming SBc sub-luminous galaxy. We detect an object consistent with being a point source within the astrometric uncertainty of 0.018 arcseconds of the position of the supernova. The object is located inside a star-forming region and is at least one magnitude 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. | |
| dc.description | 12 pages, 2 figures, AASTeX v5.02 accepted for publication in ApJ Letters | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0009014 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0009014 | |
| dc.identifier | Astrophys.J. 542 (2000) L89-L93 | |
| dc.identifier | doi:10.1086/312942 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/1591 | |
| dc.subject | Astrophysics | |
| dc.title | HST/STIS Imaging of the Host Galaxy of GRB980425/SN1998bw | |
| dc.type | text |