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Volumn 67, Issue 2, 2003, Pages

r-modes in accreting neutron stars with magnetoviscous boundary layers

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; CALCULATION; DYNAMICS; ELECTROMAGNETIC FIELD; ELECTRON; GRAVITY; MASS; MATHEMATICAL ANALYSIS; MATHEMATICAL MODEL; NEUTRON; VORTEX MOTION; X RAY ANALYSIS;

EID: 0037438312     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevD.67.024032     Document Type: Article
Times cited : (27)

References (67)
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  • 13
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    • (1988) Timing Neutron Stars , pp. 457
    • Sauls, J.A.1
  • 29
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    • P. Arras, E.E. Flanagan, S.M. Morsink, A.K. Schenk, S.A. Teukolsky, and I. Wasserman, astro-ph/0202345
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    • M. van der Klis, astro-ph/9710016
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    • Relativistic Astrophysics, edited by J. Craig Wheeler and Hugo Martel, (AIP, Melville, NY)
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    • (2001) AIP Conf. Proc. No. 586
    • Wagoner, R.V.1    Hennawi, J.F.2    Liu, J.3
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    • J. Heyl, astro-ph/0206174
    • J. Heyl, astro-ph/0206174.
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    • P.G. Jonker, M. Méndez, and M. van der Klis, astro-ph/0204113
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    • note
    • The code that generated the cycles used quality step-size control during the heating and spindown phases of the evolution. To speed up the code, once the cycle turned the lower right corner and the cooling phase had begun (indicated by the angular velocity reaching its minimum value and not changing) the code extrapolated to get the cooling and spinup phase of the curves. This was found to give the same cycles as using quality step-size control thoughout the evolution, except it makes the lower left corner of the cycles turn too sharply.
  • 67
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    • N. Andersson, D.I. Jones, and K.D. Kokkotas, astro-ph/0111582
    • N. Andersson, D.I. Jones, and K.D. Kokkotas, astro-ph/0111582.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.