Relativistic Wind Bubbles and Afterglow Signatures

Highly magnetized, rapidly rotating compact objects are widely argued to be central energy sources of gamma-ray bursts (GRBs). After the GRB, such a magnetar-like object may directly lose its rotational energy through some magnetically driven processes, which produce an ultrarelativistic wind domina...

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Veröffentlicht in:	The Astrophysical journal 2004-05, Vol.606 (2), p.1000-1005
1. Verfasser:	Dai, Z. G
Format:	Artikel
Sprache:	eng
Online-Zugang:	Volltext bestellen
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