Stellar winds and neutron star masses in two new eclipsing highly absorbed HMXB

Details Stellar winds and neutron star masses in two new eclipsing highly absorbed HMXB Stellar winds and neutron star masses in two new eclipsing highly absorbed HMXB

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005xmm..prop..211w&link_type=abstract

XMM-Newton Proposal ID #04056401

Computer Science

White Dwarf Binaries, Neutron Star Binaries, Cataclysmic Variables, Ulxs, Black Holes, Igr J17252-3616, Xmm-Newton Proposal 04056401

Scientific paper

Two of the strongly absorbed super-giant HMXB discovered by INTEGRAL are eclipsing systems. This very rare property allows a comprehensive study of the dynamics and of the stellar winds in those systems. The aim of this proposal is to obtain quantitative constraints on the ionisation, density and clumping of the stellar wind along the orbit and to measure the masses of the neutron stars.

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