Using the X-ray morphology of young supernova remnants to constrain explosion type, ejecta distribution, and chemical mixing

Astrophysical Journal

Volumn 732, Issue 2, 2011, Pages

  Lopez, Laura A ^a   Ramirez Ruiz, Enrico ^a   Huppenkothen, Daniela ^b   Badenes, Carles ^c,d   Pooley, David A ^e  

^a UNIVERSITY OF CALIFORNIA   (United States)

^b UNIVERSITY OF AMSTERDAM   (Netherlands)

^c TEL AVIV UNIVERSITY   (Israel)

^d WEIZMANN INSTITUTE OF SCIENCE   (Israel)

^e Eureka Scientific Inc   (United States)

Author keywords

ISM: supernova remnants; methods: data analysis; techniques: image processing; X rays: ISM

Indexed keywords

EID: 79955659608     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/732/2/114     Document Type: Article

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