Other
Scientific paper
Dec 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aas...19911202b&link_type=abstract
American Astronomical Society, 199th AAS Meeting, #112.02; Bulletin of the American Astronomical Society, Vol. 33, p.1478
Other
Scientific paper
Chandra HETG observations of the bright eclipsing contact binary 44 Boo show X-ray line profiles which are Doppler-shifted by orbital motions. The observation continuously covers 2.56 epochs. Although significant variability is found in the light curve, no clear eclipses are observed. The phase-binned line profiles, in conjunction with the X-ray light curve, constrain the coronal structures to be localized at high latitude. These observations demonstrate the power of the X-ray Doppler imaging technique. Studies of other contact binaries, and studies of RS CVn systems with future X-ray spectrometers are discussed.
Brickhouse Nancy S.
Dupree Andrea K.
Young Paul R.
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