Absorption and Abundances in the Ultracompact Binary 4U 0614+091

Details Absorption and Abundances in the Ultracompact Binary 4U 0614+091 Absorption and Abundances in the Ultracompact Binary 4U 0614+091

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008cxo..prop.2738c&link_type=abstract

Chandra proposal ID #10910054

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We propose to study compositions and structures of inter- and circumstellar matter using HETGS observations of the X-ray binary 4U 0614+091. We will test the TBNEW absorption model developed for XSPEC from our absorption studies for O K, Fe L, and Ne K, compare abundances for O II/III and Ne II/III with the other sample, obtain Ne/O abundance ratio and compare with other binaries, specifically ultra-compacts, measure EWs in line absorption from Ne IX, O VIII, O VII ions to characterize the hot ISM gas toward the anti-GC region

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