Sie befinden Sich nicht im Netzwerk der Universität Paderborn. Der Zugriff auf elektronische Ressourcen ist gegebenenfalls nur via VPN oder Shibboleth (DFN-AAI) möglich. mehr Informationen...
We present broadband observations of the afterglow and environment of the short GRB 111020A. An extensive X-ray light curve from Swift/XRT, XMM-Newton, and Chandra, spanning ~100 s to 10 days after the burst, reveals a significant break at delta t [approximate] 2 days with pre- and post-break decline rates of alpha [sub x.1] [approximate] -0.78 and alpha [sub x.2] -1.7, respectively. Our observations demonstrate that a growing fraction of short gamma-ray bursts (GRBs) are collimated, which may lead to a true event rate of [> or ~]100-1000 Gpc[sup -3] yr[sup -1], in good agreement with the NS-NS merger rate of [approximate]200-3000 Gpc[sup -3] yr[sup -1]. The consistency is promising for coincident short GRB-gravitational wave searches in the forthcoming era of Advanced LIGO/VIRGO.