Evaporation of Companions in VLMXBs and in Binary Millisecond Pulsars

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X-Ray Binaries and Recycled Pulsars

Part of the book series: NATO ASI Series ((ASIC,volume 377))

Abstract

The principles underlying the process of formation of a wind from a stellar atmosphere by external heating are applied to binary companions of neutron stars (NSs) which are being heated by radiation from the NS in Very-Low-Mass X-ray Binaries (VLMXBs) and in binary millisecond pulsar (BMP) systems. Among others, the possibilities of companion evaporation and of self-excited X-ray systems is discussed. The fast changes in the binary period of the ”windy” BMP 1957+20 and the nature of the newly discovered ”windy” BMP 1744-24A are discussed as well.

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© 1992 Springer Science+Business Media Dordrecht

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Shaham, J. (1992). Evaporation of Companions in VLMXBs and in Binary Millisecond Pulsars. In: van den Heuvel, E.P.J., Rappaport, S.A. (eds) X-Ray Binaries and Recycled Pulsars. NATO ASI Series, vol 377. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-2704-2_33

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  • DOI: https://doi.org/10.1007/978-94-011-2704-2_33

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-5198-9

  • Online ISBN: 978-94-011-2704-2

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