The importance of magnetic-field-oriented thermal conduction in the interaction of SNR shocks with interstellar clouds

Astrophysical Journal

Volumn 678, Issue 1, 2008, Pages 274-286

  Orlando, S ^a,c   Bocchino, F ^a,c   Reale, F ^b,c,d   Peres, G ^b,c,d   Pagano, P ^b  

^a INAF OSSERVATORIO ASTRONOMICO DI PALERMO   (Italy)

^b UNIVERSITY OF PALERMO   (Italy)

^c Consorzio COMETA ^*  (Italy)

^d INAF OSSERVATORIO ASTROFISICO DI TORINO   (Italy)

Author keywords

Conduction; ISM: clouds; ISM: magnetic fields; MHD; Shock waves; Supernova remnants

Indexed keywords

EID: 43949119091     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/529420     Document Type: Article

References (35)