A stellar wind bubble coincident with the anomalous X-ray pulsar 1E 1048.1-5937: Are magnetars formed from massive progenitors?

Astrophysical Journal

Volumn 620, Issue 2 II, 2005, Pages

  Gaensler, B M ^a   Mcclure Griffiths, N M ^b   Oey, M S ^c   Haverkorn, M ^a   Dickey, J M ^d   Green, A J ^e  

^a HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^b CSIRO   (Australia)

^c UNIVERSITY OF MICHIGAN   (United States)

^d UNIVERSITY OF TASMANIA   (Australia)

^e UNIVERSITY OF SYDNEY   (Australia)

Author keywords

ISM: bubbles; ISM: individual (GSH 288.3 0.5 28); Pulsars: individual (1E 1048.1 5937); Radio lines: ISM; Stars: neutron; Stars: winds, outflows

Indexed keywords

EID: 17044425952     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/428725     Document Type: Article

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