Computer Science
Scientific paper
Sep 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008cxo..prop.2533o&link_type=abstract
Chandra proposal ID #10200468
Computer Science
Scientific paper
The observed correlation between X-ray and radio luminosities for active stars suggests a common coronal energy reservoir from which both processes (particle acceleration for radio emission and plasma heating for X-ray emission) draw. There is a discrepancy of four orders of magnitude in L_X/L_R for very low mass stars compared to active stars, but radio variability from a different emission mechanism may complicate the interpretation. We propose to obtain X-ray and radio observations of a radio-bright close binary, LP349-25, to explore the L_X/L_R relationship for this object with apparently constant radio emission.
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