Spectroscopic distance estimates for fourteen faint red LHS and NLTT stars

Details Spectroscopic distance estimates for fourteen faint red LHS and NLTT stars Spectroscopic distance estimates for fourteen faint red LHS and NLTT stars

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001a%26a...370..967j&link_type=abstract

Astronomy and Astrophysics, v.370, p.967-973 (2001)

Astronomy and Astrophysics

Astrophysics

11

Stars: Distances, Stars: Late Type, Galaxy: Solar Neighbourhood

Scientific paper

Spectroscopic observations were carried out of potential nearby high proper motion stars taken from Luyten's LHS and NLTT catalogues. The purpose was to obtain a first distance estimate for hitherto neglected nearby candidates. The resulting spectra for fourteen stars are presented and discussed. The sample comprises eleven M dwarfs and three M subdwarfs having spectroscopic distances from 17 pc to 160 pc.

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