Bursting SN 1996cr's bubble: Hydrodynamic and X-ray modelling of its circumstellar medium

Monthly Notices of the Royal Astronomical Society

Volumn 407, Issue 2, 2010, Pages 812-829

  Dwarkadas, V V ^a   Dewey, D ^b   Bauer, F ^c,d,e  

^a UNIVERSITY OF CHICAGO   (United States)

^b MASSACHUSETTS INSTITUTE OF TECHNOLOGY   (United States)

^c Center for Extrasolar Planetary Studies   (United States)

^d PONTIFICIA UNIVERSIDAD CATÓLICA DE CHILE   (Chile)

^e Columbia University ^*  (United States)

Author keywords

Circumstellar matter; Methods: numerical; Stars: winds, outflows; Supernovae: individual: SN 1996cr; Techniques: spectroscopic; X rays: individual: SN 1996cr

Indexed keywords

NUMERICAL METHODS; SHOCK WAVES; SUPERNOVAE;

CIRCUMSTELLAR; CIRCUMSTELLAR MATTERS; METHOD: NUMERICAL; SIMULATED SPECTRA; STARS: WINDS OUTFLOWS; SUPERNOVA: INDIVIDUAL: SN 1996CR; SUPERNOVAE: INDIVIDUAL: SN 1987A; TECHNIQUES: SPECTROSCOPIC; X-RAY: INDIVIDUAL: SN 1996CR; X-RAYS: INDIVIDUAL;

HYDRODYNAMICS;

EID: 77956413037     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2010.16966.x     Document Type: Article

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