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Volumn 582, Issue 1 I, 2003, Pages 347-351

Pseudo-Newtonian potentials to describe the temporal effects on relativistic accretion disks around rotating black holes and neutron stars

Author keywords

Accretion, accretion disks; Black hole physics; Gravitation; Relativity

Indexed keywords


EID: 0042763003     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/344574     Document Type: Article
Times cited : (29)

References (17)


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.