Two-dimensional magnetohydrodynamic numerical simulations of magnetic reconnection triggered by a supernova shock in the interstellar medium: Generation of X-ray gas in the Galaxy

Astrophysical Journal

Volumn 551, Issue 1 PART 1, 2001, Pages 312-332

  Tanuma, Syuniti ^a,b,c   Yokoyama, Takaaki ^b   Kudoh, Takahiro ^b   Shibata, Kazunari ^d  

^a UNIVERSITY OF TOKYO   (Japan)

^b NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^c NAGOYA UNIVERSITY   (Japan)

^d KYOTO UNIVERSITY   (Japan)

Author keywords

Galaxy: Structure; ISM; ISM: Kinematics and dynamics; ISM: Magnetic fields; Methods: Numerical; MHD; X rays

Indexed keywords

EID: 0035836896     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/320058     Document Type: Article

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