Spectroscopic distance estimates for fourteen faint red LHS and NLTT stars
- H. Jahreiß
- R. Scholz
- H. Meusinger
- I. Lehmann
DOIAbstract
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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