The imprint of a symbiotic binary progenitor on the properties of Kepler's supernova remnant

Astronomy and Astrophysics

Volumn 537, Issue , 2012, Pages

  Chiotellis, A ^a   Schure, K M ^a,b   Vink, J ^a,c  

^a UTRECHT UNIVERSITY   (Netherlands)

^b UNIVERSITY OF OXFORD   (United Kingdom)

^c UNIVERSITY OF AMSTERDAM   (Netherlands)

Author keywords

Binaries: symbiotic; Hydrodynamics; ISM: supernova remnants; Supernovae: individual: SN1604

Indexed keywords

BINARIES: SYMBIOTIC; BLAST WAVES; BOW SHOCKS; CIRCUMSTELLAR; INITIAL MASS; INTERSTELLAR MEDIUMS; ISM: SUPERNOVA REMNANTS; MORPHOLOGICAL PROPERTIES; SHELL FORMATION; SPATIAL VELOCITY; SUPERNOVA REMNANTS; SUPERNOVAE: INDIVIDUAL; WHITE DWARFS;

EXPLOSIVES; FLUID DYNAMICS; HYDRODYNAMICS;

STARS;

EID: 84856153861     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201014754     Document Type: Article

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