Cr-K emission line as a constraint on the progenitor properties of supernova remnants

Astrophysical Journal

Volumn 766, Issue 1, 2013, Pages

  Yang, X J ^a,b   Tsunemi, H ^c   Lu, F J ^d   Li, Aigen ^b   Xiang, F Y ^a,b   Xiao, H P ^a   Zhong, J X ^a  

^a XIANGTAN UNIVERSITY   (China)

^b UNIVERSITY OF MISSOURI   (United States)

^c OSAKA UNIVERSITY   (Japan)

^d INSTITUTE OF HIGH ENERGY PHYSICS   (China)

Author keywords

ISM: individual objects (Tycho, Kepler, W49B, N103B, Cas A, G344.7 0.1, 3C397, 0519?69.0); ISM: supernova remnants

Indexed keywords

EID: 84875030493     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/766/1/44     Document Type: Article

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