This site uses cookies. By continuing to use this site you agree to our use of cookies. To find out more, see our Privacy and Cookies policy.

The Rates of Hypernovae and Gamma-Ray Bursts: Implications for Their Progenitors

, , , , and

Published 2004 April 23 © 2004. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Ph. Podsiadlowski et al 2004 ApJ 607 L17 DOI 10.1086/421347

1538-4357/607/1/L17

Abstract

A critical comparison of estimates for the rates of hypernovae (HNe) and gamma-ray bursts (GRBs) is presented. Within the substantial uncertainties, the estimates are shown to be quite comparable and give a galactic rate of 10-6 to 10-5 yr-1 for both events. These rates are several orders of magnitude lower than the rate of core-collapse supernovae, suggesting that the evolution leading to an HN/GRB requires special circumstances, very likely due to binary interactions. Various possible binary channels are discussed, and it is shown that these are generally compatible with the inferred rates.

Export citation and abstract BibTeX RIS

Please wait… references are loading.
10.1086/421347