Eclipsing Binary X-Ray Halos and Interstellar Grain Properties

Details Eclipsing Binary X-Ray Halos and Interstellar Grain Properties Eclipsing Binary X-Ray Halos and Interstellar Grain Properties

Sep 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999cxo..prop..243g&link_type=abstract

Chandra Proposal ID #01400046

Computer Science

Chandra Proposal Id #01400046

Scientific paper

Study of the X-ray scattered halo around obscured Galactic X-ray sources can provide insights into the size, density, composition and spatial distribution of interstellar grains. Eclipsing X-ray binary systems offer unique advantages, as the evolution of the halo following an abrupt eclipse depends on the distance and distribution of clouds. A high-resolution spectrum will further provide rich information on the interstellar matter composition.

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