High-resolution simulations of the plunging region in a pseudo-Newtonian potential: Dependence on numerical resolution and field topology

Astrophysical Journal

Volumn 566, Issue 1 I, 2002, Pages 164-180

  Hawley, John F ^a   Krolik, Julian H ^b  

^a UNIVERSITY OF VIRGINIA   (United States)

^b JOHNS HOPKINS UNIVERSITY   (United States)

Author keywords

Accretion, accretion disks; Black hole physics; Instabilities; MHD

Indexed keywords

EID: 0000420183     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/338059     Document Type: Article

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