Lithium in an Extreme Halo Star
Abstract
Echelle spectra show that BD +3°740 is an extreme Population II dwarf with a logarithmic metallicity [Fe/H] ≈ -2.9, a space velocity |vLSR| ≈ 210 km s-1, and an effective temperature Te ≈ 6240K. Small corrections of the star's observed colors for interstellar reddening are derived from the observed interstellar D lines. The equivalent width Wλ = 17±3 mÅ of the Li I λ6707 line gives an abundance Li/H = (1.2±0.5)×10-10, in agreement with previous results for two other extreme halo stars.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- March 1988
- DOI:
- 10.1086/185115
- Bibcode:
- 1988ApJ...326L..23H
- Keywords:
-
- Dwarf Stars;
- Lithium;
- Metallicity;
- Stellar Composition;
- Stellar Spectra;
- D Lines;
- Interstellar Extinction;
- Spectral Line Width;
- Stellar Temperature;
- Astrophysics;
- STARS: ABUNDANCES;
- STARS: POPULATION II