Oxygen abundances from infrared OH lines
- 1 July 2001
- journal article
- Published by Elsevier in New Astronomy Reviews
- Vol. 45 (8) , 529-531
- https://doi.org/10.1016/s1387-6473(01)00118-x
Abstract
No abstract availableKeywords
This publication has 8 references indexed in Scilit:
- The Importance of F[CLC]e[/CLC] [CSC]i[/CSC] as a Continuous Opacity Source in the Solar AtmosphereThe Astrophysical Journal, 2001
- The effective temperature scale of giant stars (F0–K5)Astronomy and Astrophysics Supplement Series, 1999
- Erratum: “Oxygen in Unevolved Metal-poor Stars from Keck Ultraviolet HIRES Spectra” [[URL ADDRESS="http://www.journals.uchicago.edu/cgi-bin/resolve?AJ980326" STATUS="OKAY"]Astron. J. [BF]117[/BF], 492 (1999)[/URL]]The Astronomical Journal, 1999
- Oxygen Abundances in Unevolved Metal‐poor Stars from Near‐Ultraviolet OH LinesThe Astrophysical Journal, 1998
- Shallow mixing in the solar photosphere inferred from revised beryllium abundancesNature, 1998
- Isochrones for Hydrogen‐burning Globular Cluster Stars. III. From the Sun to the Globular ClustersThe Astrophysical Journal, 1997
- The Oxygen Abundances in Halo Dwarfs. I. HD 103095The Astronomical Journal, 1996
- Spectral line parameters for the A2∑-X2Π(0,0) band of OH for atmospheric and high temperaturesJournal of Quantitative Spectroscopy and Radiative Transfer, 1981