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

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

May 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004a%26at...23..497g&link_type=ejournal

Astronomical and Astrophysical Transactions, vol. 23, Issue 5, p.497-498

Astronomy and Astrophysics

Astrophysics

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