Simultaneous X-Ray and Photometric Observations of the Flare Star YZ CMi
DOI: 10.1007/3-540-16763-3_180
Bibcode: 1986LNP...254..228D
Doyle, J. G.; Butler, C. J.
United Kingdom
Abstract
Broad-band photometric observations of YZ CMi show a 1.2 magnitude U-band flare, however, simultaneous X-ray observations from EXOSAT show no detectable increase. It is suggested that the energy was dissipated before reaching the corona. Two long duration U-band enhancements detected during the optical monitoring may have been the result of back-heating from an enhanced coronal X-ray flux.
1986
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Cool Stars, Stellar Systems and the Sun
Exosat
0