Low Mass X-ray Binary As the Progenitor of PSR J1713+0747

Details Low Mass X-ray Binary As the Progenitor of PSR J1713+0747 Low Mass X-ray Binary As the Progenitor of PSR J1713+0747

2005-12-22

arxiv.org/abs/astro-ph/0512558v2

Publ.Astron.Soc.Jap. 58 (2006) 153-158

Astronomy and Astrophysics

Astrophysics

8 pages, 4 figures, accepted for publication in PASJ

Scientific paper

We have calculated the evolution of low-mass X-ray binaries that leads to the formation of the binary radio pulsars like PSR J1713+0747. We show that the mass transfer is most likely to be nonconservative, due to unstable disk accretion, to account for the mass of PSR J1713+0747, which is close to its initial value. We assume that part of the lost material from the binary may form a circumbinary disk, and find that it can significantly influence the mass transfer processes. We briefly discuss the implications of the circumbinary disks on the evolution of low-mass X-ray binaries and the formation of low-mass binary pulsars.

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