RGS observation of HD101088, a young binary accreting from a transition disk

Details RGS observation of HD101088, a young binary accreting from a transition disk RGS observation of HD101088, a young binary accreting from a transition disk

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010xmm..prop...84g&link_type=abstract

XMM-Newton Proposal ID #06720801

Physics

Stars, White Dwarfs, Solar System, Hd101088

Scientific paper

HD101088 is a young binary accreting from a tenuous circumprimary and/or circumsecondary disk despite the apparent lack of a massive dusty circumbinary disk. We propose to observe it with RGS with an exposure of 60 ks to detect the emission lines from the O VII He-like ion and look for potential high-density plasma at the base of the accretion flows. HD101088 is a unique target to investigate the physical properties of the accreting gas and the stellar corona after the dissipation of the dust disk.

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