On the stellar X-ray content of the Open Cluster Remnant NGC 1901

Details On the stellar X-ray content of the Open Cluster Remnant NGC 1901 On the stellar X-ray content of the Open Cluster Remnant NGC 1901

Oct 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009xmm..prop....2l&link_type=abstract

XMM-Newton Proposal ID #06500201

Physics

Stars, White Dwarfs, Solar System, Ngc 1901

Scientific paper

Open Cluster Remnants (OCRs) are poorly populated groups of stars in an advanced stage of the evolution of open clusters. They are especially rich in late-type stars and binary systems of stars, of which a fraction is expected to be interacting binaries (RS CVn, cataclysmic variables, and low-mass X-ray binaries). We propose to investigate the X-ray content of the OCR NGC 1901, looking for signatures of accreting/interacting binary systems and active stars in order to put constraints on the evolutionary models describing the final stages of star clusters.

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