Some Aspects of Low-Mass Close Binary Models for Bright Galactic Bulge X-Ray Sources and 4U1626-67

Details Some Aspects of Low-Mass Close Binary Models for Bright Galactic Bulge X-Ray Sources and 4U1626-67 Some Aspects of Low-Mass Close Binary Models for Bright Galactic Bulge X-Ray Sources and 4U1626-67

Mar 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26a....95l..11k&link_type=abstract

Astronomy and Astrophysics, Vol. 95, P. L11, 1981

Astronomy and Astrophysics

Astrophysics

20

Scientific paper

Assuming that gravitational radiation loss is the driving mechanism for mass transfer in the brightest galactic bulge X-ray sources various conditions are examined in order to obtain the highest possible mass-transfer rates.
It is found that even if angular momentum losses from the disk are taken into account, only in case of a degenerate star as secondary the mass-transfer rate can reach values as high as are required to explain the highest observed luminosities of these sources. The 2500 sec orbital period of 4U 1626 - 67 seems to require a hydrogen-rich low-mass degenerate secondary star.

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