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

Author： Guseinov O. H.   Allakhverdiev A. O.   Tagieva Sevinç   Taşki˙n Özgür  

Publisher： Taylor & Francis Ltd

ISSN： 1055-6796

Source： Astronomical and Astrophysical Transactions, Vol.23, Iss.5, 2004-10, pp. : 497-498

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

Previous Menu Next

Abstract

Related content

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

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

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

Taylor & Francis Ltd

Access to resources Recommend Favorite

Infrared Observations of High-Mass X-Ray Binaries

By Kaper L.  

Astrophysics and Space Science, Vol. 255, Iss. 1-2, 1997-01 ,pp. : 199-204

Springer Publishing Company

Access to resources Recommend Favorite

The search for high-mass X-ray binaries in the Phoenix dwarf galaxy

By Bartlett E. S.   Coe M. J.   Haberl F.   McBride V. A.   Corbet R. H. D.  

Monthly Notices of the Royal Astronomical Society, Vol. 422, Iss. 3, 2012-05 ,pp. : 2302-2313

Oxford University Press

Access to resources Recommend Favorite

Accreting magnetars: a new type of high-mass X-ray binaries?

By Reig P.   Torrejón J. M.   Blay P.  

Monthly Notices of the Royal Astronomical Society, Vol. 425, Iss. 1, 2012-09 ,pp. : 595-604

Oxford University Press

Access to resources Recommend Favorite

High-mass X-ray binaries and the spiral structure of the host galaxy

By Shtykovskiy P.   Gilfanov M.  

Astronomy Letters, Vol. 33, Iss. 5, 2007-05 ,pp. : 299-308

MAIK Nauka/Interperiodica

Access to resources Recommend Favorite