STIS/Spectroscopy of the Brown Dwarf Gl229B

Details STIS/Spectroscopy of the Brown Dwarf Gl229B STIS/Spectroscopy of the Brown Dwarf Gl229B

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997hst..prop.7130s&link_type=abstract

HST Proposal ID #7130

Physics

Hst Proposal Id #7130

Scientific paper

This proposal requests high-resolution spectroscopy of GL229B, a brown
dwarf, covering the spectral region from 0.5-1.0mu. Due to the its faint
magnitude {mv > 22} and separation { 7.5 arcsec} from the primary
star GL229A {mv 8.12}, only ground-based infrared observations of
GL229B have been reported and used to model the temperature and mass.

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