THE AFTERGLOWS OF<i>SWIFT</i>-ERA GAMMA-RAY BURSTS. II. TYPE I GRB VERSUS TYPE II GRB OPTICAL AFTERGLOWS

А. Канн, Д.; Klose, S.; Zhang, Bing; Covino, S.; Butler, N.; Malesani, D.; Nakar, Ehud; C. Wilson, A.; A. Antonelli, L.; Chincarini, G.; E. Cobb, B.; D’Avanzo, P.; D’Elia, V.; Della Valle, M.; Ferrero, P.; Fugazza, D.; Gorosabel, J.; L. Israel, G.; Mannucci, F.; Piranomonte, S.; Schulze, S.; Stella, L.; Tagliaferri, G.; Wiersema, K.

doi:10.1088/0004-637x/734/2/96

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THE AFTERGLOWS OFSWIFT-ERA GAMMA-RAY BURSTS. II. TYPE I GRB VERSUS TYPE II GRB OPTICAL AFTERGLOWS

Published in The Astrophysical Journal • Jun 1, 2011

Authors:

Д. А. Канн

S. Klose

Bing Zhang

Abstract

Gamma-ray bursts (GRBs) have been separated into two classes, originally along the lines of duration and spectral properties, called "short/hard" and "long/soft." The latter have been conclusively linked to the explosive deaths of massive stars, while the former are thought to result from the merger...

Subject

Afterglow

Gamma-ray burst

Physics

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