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Paper detail

Interacting compact binaries: modeling mass transfer in eccentric systems

We discuss mass transfer in eccentric binaries containing a white dwarf and a neutron star (WD--NS binaries). We show that such binaries are produced from field binaries following a series of mass transfer episodes that allow the white dwarf to form before the neutron star. We predict the orbital properties of binaries similar to the observed WD--NS binary J1141+6545, and show that they will undergo episodic mass transfer from the white dwarf to the neutron star. Furthermore, we describe oil-on-water, a two-phase SPH formalism that we have developed in order to model mass transfer in such binaries.

preprint2011arXivOpen access
Ross P. ChurchMelvyn B. DaviesAlexey BobrickChristopher A. Tout
astro-ph.HE
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Ross P. ChurchMelvyn B. DaviesAlexey BobrickChristopher A. Tout

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