LSR 1610-0040: The First Early-Type L Subdwarf
Abstract
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 Msolar).
- Publication:
-
The Astrophysical Journal
- Pub Date:
- July 2003
- DOI:
- arXiv:
- arXiv:astro-ph/0305554
- Bibcode:
- 2003ApJ...591L..49L
- Keywords:
-
- Galaxy: Stellar Content;
- Stars: Fundamental Parameters;
- Stars: Late-Type;
- Stars: Low-Mass;
- Brown Dwarfs;
- Stars: Subdwarfs;
- Astrophysics
- E-Print:
- To appear in The Astrophysical Journal Letters