Orbital evolution of binaries with ultra-rapid pulsars

Details Orbital evolution of binaries with ultra-rapid pulsars Orbital evolution of binaries with ultra-rapid pulsars

Nov 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...265...65e&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 265, no. 1, p. 65-70.

Astronomy and Astrophysics

Astrophysics

6

Binary Stars, Pulsars, Stellar Mass Ejection, Stellar Orbits, Angular Momentum, Mass Transfer, Stellar Evolution, Stellar Mass Accretion, Stellar Winds, X Ray Binaries

Scientific paper

For the case of large evaporation mass loss efficiency, binary evolution with ultra-rapid pulsar has been investigated. It is proposed that the accretion and evaporation phases will alter. In the frame of this scenario, it is possible to explain the increase of orbital separation of the low-mass X-ray binary X1822-371. Application the evaporation scenario to PSR 1957 + 20 and MXB 1820-30 will be discussed.

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