Unveiling the spatial structure of the overionized plasma in the supernova remnant W49B

Monthly Notices of the Royal Astronomical Society

Volumn 415, Issue 1, 2011, Pages 244-250

  Zhou, Xin ^a,b   Miceli, Marco ^b,c   Bocchino, Fabrizio ^b   Orlando, Salvatore ^b   Chen, Yang ^a  

^a NANJING UNIVERSITY   (China)

^b INAF OSSERVATORIO ASTROFISICO DI TORINO   (Italy)

^c UNIVERSITY OF PALERMO   (Italy)

Author keywords

Hydrodynamics; ISM: individual objects: G43.3 0.2; ISM: individual objects: W49B; ISM: supernova remnants; Methods: numerical

Indexed keywords

COOLING; FIGHTER AIRCRAFT; MIXING; NUMERICAL METHODS; PLASMA DIAGNOSTICS; SUPERNOVAE;

CIRCUMSTELLAR; ISM: INDIVIDUAL OBJECT: G43.3-0.2; ISM: INDIVIDUAL OBJECT: W49B; ISM: INDIVIDUAL OBJECTS; ISM: SUPERNOVA REMNANTS; METHOD: NUMERICAL; SPATIAL STRUCTURE; SUPERNOVA REMNANTS; THERMAL CONDUCTION;

HYDRODYNAMICS;

EID: 79960121629     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2011.18695.x     Document Type: Article

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