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Volumn 582, Issue 1 I, 2003, Pages 347-351
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Pseudo-Newtonian potentials to describe the temporal effects on relativistic accretion disks around rotating black holes and neutron stars
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Author keywords
Accretion, accretion disks; Black hole physics; Gravitation; Relativity
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Indexed keywords
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EID: 0042763003
PISSN: 0004637X
EISSN: 15384357
Source Type: Journal
DOI: 10.1086/344574 Document Type: Article |
Times cited : (29)
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References (17)
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