Near-Infrared Adaptive Optics Spectroscopy of Binary Brown Dwarf HD 130948B and HD 130948C

Details Near-Infrared Adaptive Optics Spectroscopy of Binary Brown Dwarf HD 130948B and HD 130948C Near-Infrared Adaptive Optics Spectroscopy of Binary Brown Dwarf HD 130948B and HD 130948C

Jun 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003iaus..211..263g&link_type=abstract

Brown Dwarfs, Proceedings of IAU Symposium #211, held 20-24 May 2002 at University of Hawaii, Honolulu, Hawaii. Edited by Eduard

Physics

Optics

Scientific paper

We present near-infrared spectroscopy of low-mass companions in the HD 130948 system (Goto et al. 2002a). Adaptive optics on the Subaru Telescope allowed for spectroscopy of the individual components of the 0.13 arcs binary system. Based on a direct comparison with a series of template spectra, we determined the spectral types of HD 130948B and C to be L4 ± 1. We find they are most likely a binary brown dwarf system.

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