Report

GRB 130427A: A Nearby Ordinary Monster

Science  21 Nov 2013:

DOI: 10.1126/science.1242279

You are currently viewing the abstract.

View Full Text

Via your Institution

Log in through your institution

Log in through your institution


This article has a correction. Please see:

Abstract

Long-duration Gamma-Ray Bursts (GRBs) are an extremely rare outcome of the collapse of massive stars, and are typically found in the distant Universe. Because of its intrinsic luminosity (L ∼ 3 × 1053 erg s−1) and its relative proximity (z = 0.34), GRB 130427A was a unique event that reached the highest fluence observed in the γ-ray band. Here we present a comprehensive multiwavelength view of GRB 130427A with Swift, the 2-m Liverpool and Faulkes telescopes and by other ground-based facilities, highlighting the evolution of the burst emission from the prompt to the afterglow phase. The properties of GRB 130427A are similar to those of the most luminous, high-redshift GRBs, suggesting that a common central engine is responsible for producing GRBs in both the contemporary and the early Universe and over the full range of GRB isotropic energies.

View Full Text

Related Content