Flare Activity and Coronal Heating on the Active Flare Star Binary UV Ceti

Details Flare Activity and Coronal Heating on the Active Flare Star Binary UV Ceti Flare Activity and Coronal Heating on the Active Flare Star Binary UV Ceti

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000cxo..prop..552a&link_type=abstract

Chandra Proposal ID #02200375

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Chandra Proposal Id #02200375

Scientific paper

Coronal heating on active stars has been related to magnetic flare activity explicitly seen in these stars, or to microflaring concepts accessible through flare energy distribution statistics and coronal parameters (temperatures, emission measure distributions, densities, mass flows). We propose to test these concepts in the extremely variable flare star binary UV Cet, requesting an 80 ks exposure that will provide information on overall coronal parameters, flare statistics, and flare heating mechanisms. A coordinated VLA observation is planned. This exposure will probe two apparently identical stars at the same time. Their separation of 1" does not split the spectral lines, while the 0th order image in the proposed LETGS/HRC-S will clearly resolve the binary.

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