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Volumn 5, Issue 4, 2007, Pages 457-462

A remark about possible unity of the neutron star and black hole high frequency QPOs

Author keywords

Accretion; Accretion discs; Binaries; Neutron; Stars; X rays

Indexed keywords


EID: 36749098030     PISSN: 18951082     EISSN: 16443608     Source Type: Journal    
DOI: 10.2478/s11534-007-0039-0     Document Type: Article
Times cited : (18)

References (21)
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  • 18
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    • accepted,2007,Preprint arXiv:astro-ph/0705.0793
    • T. Belloni, J. Homan, S. Motta, E. Ratti and M. Mendez: "RossiXTE monitoring of 4U 1636-53:I. Long-term evolution and kHz Quasi-Periodic Oscillations", Mon. Not. R. Astron. Soc., accepted,2007,Preprint arXiv:aStro-ph/0705.0793.
    • Mon. Not. R. Astron. Soc.
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    • "On a multi-resonant origin of high frequency quasiperiodic oscillations in the neutron-star X-ray binary 4U 1636-53"
    • in preparation, 2007
    • Z. Stuchlík, P. Bakala and G. Török: "On a multi-resonant origin of high frequency quasiperiodic oscillations in the neutron-star X-ray binary 4U 1636-53", in preparation, 2007.
    • Stuchlík, Z.1    Bakala, P.2    Török, G.3


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.