Eclipses and Halos in the X-Ray Pulsar 1H0253+193

Details Eclipses and Halos in the X-Ray Pulsar 1H0253+193 Eclipses and Halos in the X-Ray Pulsar 1H0253+193

Sep 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999cxo..prop..167n&link_type=abstract

Chandra Proposal ID #01910666

Computer Science

Chandra Proposal Id #01910666

Scientific paper

1H0253+193 is a hard X-ray source, situated by chance directly behind a dense nearby molecular cloud, MBM~12 (Lynds 1457). 1H0253+193 exhibits sharp, apparently complete, eclipses, lasting 1990~s and occuring every 21,800~s. These properties make this an ideal source for studying the size and chemical composition of interstellar grains via the temporal behavior of the X-ray flux resulting from dust scattering effects during the eclipse.

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