GRB 970228 Revisited: Evidence for a Supernova in the Light Curve and Late Spectral Energy Distribution of the Afterglow

1999/06/30 by Daniel E. Reichart, D. Reichart · 12 citations
Physics and Astronomy · #Afterglow #Astro and Planetary Science #Astronomy #Astrophysics #Galaxy #Gamma-ray burst #Gamma-ray bursts and supernovae #Light curve #Physics #Spectral energy distribution #Stellar, planetary, and galactic studies #Supernova #astro-ph

paper · pdf · doi:10.1086/312203

published as Astrophys.J. 521 (1999) L111-L115 · Accepted to The Astrophysical Journal (Letters), 14 pages, LaTeX

arxiv created 1999/07/30 · openalex publication_date 1999/08/20 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

At the time of its discovery, the optical and X-ray afterglow of GRB 970228 appeared to be a ringing endorsement of the previously untried relativistic fireball model of gamma-ray burst (GRB) afterglows, but now that nearly a dozen optical afterglows to GRBs have been observed, the wavering light curve and reddening spectrum of this afterglow make it perhaps the most difficult of the observed afterglows to reconcile with the fireball model. In this Letter, we argue that this afterglow's unusual temporal and spectral properties can be attributed to a supernova that overtook the light curve nearly 2 weeks after the GRB. This is the strongest case yet for a GRB/supernova connection. It strengthens the case that a supernova also dominated the late afterglow of GRB 980326 and the case that GRB 980425 is related to SN 1998bw.

Citations

• The Fading Optical Counterpart of GRB 970228, 6 Months and 1 Year Later
• Optical and Long‐Wavelength Afterglow from Gamma‐Ray Bursts
• Observations and Theoretical Implications of GRB 970228

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• Explosive Nucleosynthesis Associated with Formation of Jet‐induced Gamma‐Ray Bursts in Massive Stars
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