We report the discovery of the coolest subdwarf reported to date. The star LSR 1425+7102 was discovered in our survey for faint high proper motion stars in the northern sky. Follow-up spectroscopy revealed the star to be a very red object with the characteristic signature of M subdwarfs: strong CaH bands but relatively weaker TiO bands. The CaH molecular band at ≈6900 Å is particularly strong. By extrapolating the empirical relationship between the strength of the CaH molecular band and that of the subdwarf subtype, we conclude that LSR 1425+7102 is the first star to be discovered with spectral type sdM8.0.
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Lépine et al. (2003) studied this question.
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