The Source of X-Rays in the HR 1442 System

Details The Source of X-Rays in the HR 1442 System The Source of X-Rays in the HR 1442 System

Sep 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999cxo..prop...49w&link_type=abstract

Chandra Proposal ID #01200382

Physics

Chandra Proposal Id #01200382

Scientific paper

HR 1442 is a pair of B9 IV stars associated with the Taurus star formation region. It is also one of the brightest X-ray sources in this star formation region. ROSAT HRI observations could not resolve the pair. Ground based observations shows that one of the B stars has an infrared excess, a lithium absorption line, and may have a circumstellar disk. There is also a fainter IR-bright star nearby. We propose an HRC-I imaging observation to resolve the source(s) of the X-rays in this system. This will assist in elucidating the nature of the peculiar B star.

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