Discovery of the Coolest Extreme Subdwarf

Details Discovery of the Coolest Extreme Subdwarf Discovery of the Coolest Extreme Subdwarf

2006-03-15

arxiv.org/abs/astro-ph/0603382v1

Astrophys.J. 645 (2006) 1485-1497

Astronomy and Astrophysics

Astrophysics

19 pages, 7 figures, accepted for publication in ApJ; Figure 1 is available as a JPEG file at http://arxiv.org/PS_cache/astr

Scientific paper

10.1086/504375

We report the discovery of LEHPM 2-59 as the coolest extreme M subdwarf (esdM) found to date. Optical and near infrared spectroscopy demonstrate that this source is of later spectral type than the esdM7 APMPM 0559-2903, with the presence of strong alkali lines (including Rb I), VO absorption at 7400 A and H2O absorption at 1.4 microns. Current optical classification schemes yield a spectral type of esdM8, making LEHPM 2-59 one of only two ultracool esdMs known. The substantial space velocity of this object (V_galactic ~ -180 km/s) identifies it as a halo star. Spectral model fits to the optical and near infrared spectral data for this and four other late-type esdMs indicate that LEHPM 2-59 is the coolest esdM currently known, with Teff = 2800-3000 K and -1.5 <~ [M/H] <~ -2.0. Comparison of Teff determinations for M dwarfs and esdMs based on spectral model fits from this study and the literature demonstrate a divergence in Teff scales beyond spectral types M5/esdM5, as large as 600-800 K by types M8/esdM8. While this divergence is likely an artifact of the underlying classification scheme, it may lead to systematic errors in the derived properties of intermediate metallicity subdwarfs. We comment on the future of ultracool subdwarf classification, and suggest several ideas for addressing shortcomings in current (largely extrapolated) schemes.

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