Origin of pulsars with 0.1 s < P < 0.3 s and 5 × 105 years < τ < 107 years after the second supernova explosion in high-mass X-ray binaries

Author： Guseinov O. H.   Allakhverdiev A. O.   Tagieva Sevinç   Taşk˙in Özgür  

Publisher： Taylor & Francis Ltd

ISSN： 1055-6796

Source： Astronomical and Astrophysical Transactions, Vol.23, Iss.4, 2004-08, pp. : 385-394

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