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Spectroscopic, kinematic, and photometric data for some 200 LFT stars are presented. Eleven white dwarfs are found in the survey and two new candidates are added to a possible group of white dwarfs. Most of the remaining stars are M dwarfs of the old-disk and halo populations. The kinematic differences between these populations are reflected in the spectral lines of the halo stars where [MIHi > - 1. Key words: large proper motions - nearby stars - white dwarfs - red dwarfs
Rodgers et al. (Tue,) studied this question.