Simulating anisotropic thermal conduction in supernova remnants - II. Implications for the interstellar medium

Monthly Notices of the Royal Astronomical Society

Volumn 386, Issue 2, 2008, Pages 642-656

  Balsara, Dinshaw S ^a   Bendinelli, Anthony J ^a   Tilley, David A ^a   Massari, Andrew R ^a   Howk, J Christopher ^a  

^a UNIVERSITY OF NOTRE DAME   (United States)

Author keywords

Conduction; ISM: evolution; MHD; Supernova remnants; X rays: ISM

Indexed keywords

ANISOTROPY; INDUSTRIAL HEATING;

CONDUCTION; DENSITY FIELDS; HOT GAS; INTERSTELLAR MEDIAS; ISM:EVOLUTION; MAGNETIC FIELD STRENGTHS; RADIOACTIVE SPECIES; SUPERNOVA REMNANTS; THERMAL CONDUCTION; X RAYS: ISM;

RADIOACTIVITY;

EID: 42549086185     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2008.13121.x     Document Type: Article

References (70)