The circumstellar environment of rotating Wolf-Rayet Stars and the implications for GRB afterglows

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dc.creatorEldridge, J. J.
dc.date2006-10-13
dc.date.accessioned2026-07-07T11:04:16Z
dc.date.available2026-07-07T11:04:16Z
dc.descriptionIf Wolf-Rayet stars are the progenitors of Gamma-ray bursts (GRBs), they must rotate rapidly to produce the GRB. This rotation may effect their stellar-wind bubbles and possibly explain why so many GRB afterglows occur in a constant density medium.
dc.description2 pages, 1 figure. To appear in the proceedings of the RS GRB discussion meeting
dc.identifierhttps://arxiv.org/abs/astro-ph/0610413
dc.identifierhttp://arxiv.org/abs/astro-ph/0610413
dc.identifierPhil.Trans.Roy.Soc.Lond.A365:1255-1256,2007
dc.identifierdoi:10.1098/rsta.2006.1973
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/188836
dc.subjectAstrophysics
dc.titleThe circumstellar environment of rotating Wolf-Rayet Stars and the implications for GRB afterglows
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