X-ray emission from wide brown dwarf binaries

Details X-ray emission from wide brown dwarf binaries X-ray emission from wide brown dwarf binaries

Sep 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009cxo..prop.2759s&link_type=abstract

Chandra proposal ID #11200153

Physics

Scientific paper

Wide binary brown dwarfs offer a unique opportunity to study similarities and differences of substellar objects that were born and have evolved together. They also represent an efficient way to search for relations of brown dwarf X-ray emission with bolometric luminosity, effective temperature and mass, yielding two points in the parameter space at one shot. Only four wide binary brown dwarfs are known in various star forming regions. We have already successfully resolved one of them with Chandra, and propose here to observe all remaining three.

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