Using time variability to search for XRBs in Local GroupDwarf Galaxies

Details Using time variability to search for XRBs in Local GroupDwarf Galaxies Using time variability to search for XRBs in Local GroupDwarf Galaxies

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010xmm..prop..182c&link_type=abstract

XMM-Newton Proposal ID #06743501

Physics

White Dwarf Binaries, Neutron Star Binaries, Cataclysmic Variables, Ulxs, Black Holes, Phoenix

Scientific paper

Dwarf galaxies, both irregular and elliptical/spirals represent a key stage in the formation of galactic structures - possibly one of the earliest phases. Studies of such objects, and the formation of stars therein, is relevant to research on stellar evolution, primordial abundances and the chemical evolution of galaxies in general. Through the X-ray channel it is possible to gain significant insight into the formation of evolved binary systems and hence the underlying star formation rates (SFR) over recent epochs. In this proposal we request observations to investigate time variability amongst the proposed XRB populations of the Phoenix and NGC6822 galaxies.

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