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

Authors: O. H. Guseinov; A. O. Allakhverdiev; Sevinç Tagieva; Özgür Taki·n

Source: Astronomical and Astrophysical Transactions, Volume 23, Number 5, October 2004 , pp. 497-498(2)

Publisher: Taylor and Francis Ltd

Document Type: Research article

DOI: http://dx.doi.org/10.1080/10556790412331315806

Publication date: 2004-10-01

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