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Volumn 335, Issue 6068, 2012, Pages 561-563

Spin-down of radio millisecond pulsars at genesis

Author keywords

[No Author keywords available]

Indexed keywords

ASTROPHYSICS; COSMOLOGY; EXTRATERRESTRIAL MATTER; MAGNETOSPHERE; MASS TRANSFER; RADIO WAVE; TORQUE; X-RAY;

EID: 84856652373     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1216355     Document Type: Article
Times cited : (104)

References (37)
  • 6
    • 84922693328 scopus 로고    scopus 로고
    • note
    • The Roche lobe of a binary star is the innermost equipotential surface passing through the first Lagrangian point, L1. If a star fills its Roche lobe, the unbalanced pressure at L1 will cause mass transfer to the other star (2).
  • 7
    • 67149116783 scopus 로고    scopus 로고
    • 10.1126/science.1172740
    • A. M. Archibald et al., Science 324, 1411 (2009); 10.1126/science. 1172740.
    • (2009) Science , vol.324 , pp. 1411
    • Archibald, A.M.1
  • 8
    • 2142803437 scopus 로고    scopus 로고
    • Materials and methods are available as supporting material on
    • Materials and methods are available as supporting material on Science Online.
    • Science Online
  • 18
    • 84922746506 scopus 로고    scopus 로고
    • note
    • The magnetospheric coupling parameter, 0:5 < φ < 1:4 is a numerical factor of order unity depending on the accretion flow, the disk model, and the magnetic inclination angle of the pulsar (10, 11, 32-34).
  • 22
    • 84922727206 scopus 로고    scopus 로고
    • note
    • This "turn-off problem" has previously been debated elsewhere (13, 33, 35).
  • 28
    • 84922714913 scopus 로고    scopus 로고
    • note
    • This is the case if the pulsar spin period, P, is close to its initial spin period, P0.
  • 29


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.