Investigating the multiplicity of the L dwarf LHS 102B

Details Investigating the multiplicity of the L dwarf LHS 102B Investigating the multiplicity of the L dwarf LHS 102B

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003hst..prop.9990f&link_type=abstract

HST Proposal ID #9990

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Hst Proposal Id #9990

Scientific paper

Cycle 11 NICMOS images of LHS 102B {Program 9485} suggest that the L dwarf is a close visual binary separated by about 88 milliarcsec, which corresponds to an apparent physical separation of 0.85 AU. We will image this L dwarf with the HRC approximately one year after the NICMOS observations to confirm this probable binarity and to investigate the nature of another faint object located within 2 arcsec of LHS 102B.

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