Transient radiative winds from He-rich thermonuclear bursts

Details Transient radiative winds from He-rich thermonuclear bursts Transient radiative winds from He-rich thermonuclear bursts

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005xmm..prop..250g&link_type=abstract

XMM-Newton Proposal ID #04069002

Physics

White Dwarf Binaries, Neutron Star Binaries, Cataclysmic Variables, Ulxs, Black Holes, 4U 1728-34, 4U 1728-34, Xmm-Newton Proposal 04069002

Scientific paper

He-rich thermonuclear bursts are at present unexamined by high-sensitivity, high-spectral resolution observations. Theoretical simulations predict conditions at the peak of such bursts conducive to producing rich emission line and photoionisation edge spectra from a variety of heavy elements. We propose observations of 4U 1728-34, the only source which produces frequent He-rich bursts, in order to test for such features and also to undertake deep searches for persistent spectral features and orbital intensity modulations.

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