GRB 130427A: A Nearby Ordinary Monster


MASELLI A., MELANDRI A., NAVA L., Mundell C. G. , KAWAI N., Campana S., ...Daha Fazla

SCIENCE, cilt.343, ss.48-51, 2014 (SCI İndekslerine Giren Dergi) identifier identifier identifier

  • Cilt numarası: 343 Konu: 6166
  • Basım Tarihi: 2014
  • Doi Numarası: 10.1126/science.1242279
  • Dergi Adı: SCIENCE
  • Sayfa Sayıları: ss.48-51

Özet

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 similar to 3 x 10(53) ergs per second) and its relative proximity (z = 0.34), GRB 130427A reached the highest fluence observed in the gamma-ray band. Here, we present a comprehensive multiwavelength view of GRB 130427A with Swift, the 2-meter 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.