Computer Science
Scientific paper
Sep 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005cxo..prop.1877s&link_type=abstract
Chandra Proposal ID #07200003
Computer Science
Chandra Proposal Id #07200003
Scientific paper
2M1101926-7732383 AB is the only wide-separation brown dwarf binary known to date. Therefore it provides a unique opportunity to study in a coeval pair the influence of parameters such as mass and effective temperature on X-ray emission from young brown dwarfs. Combined with previous sensitive X-ray observations from somewhat higher-mass objects at the substellar borderline in ChaI we will be able to examine the dependence between X-ray luminosity and stellar parameters, and compare their relation to those seen in higher-mass T Tauri stars.
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