We report the discovery of LSR 1610-0040, a previously unreported r = 17.5 star with a very high proper motion, μ = 1 46 yr -1 . This very cool star ( b - i = 6.3) is found to have a peculiar spectrum that does not fit into the standard sequence of late-M dwarfs and L dwarfs. Rather, the spectrum is more typical of an ultracool subdwarf, with weak bands of TiO and no detectable VO. But because LSR 1610-0040 is so much redder than any other sdM known, and because it does not appear to fit well into the sdM sequence, we propose that LSR 1610-0040 be assigned a spectral type sdL, making it the first early-type L subdwarf known. Evidence suggests that LSR 1610-0040 is an old, metal-poor star whose mass is just above the limit of hydrogen burning ( M ≈ 0.08 M ☉ ).
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Rich et al. (2003) studied this question.
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