IMPROVED V I log( gf ) VALUES AND ABUNDANCE DETERMINATIONS IN THE PHOTOSPHERES OF THE SUN AND METAL-POOR STAR HD 84937
- 1 January 2014
- journal article
- Published by American Astronomical Society in The Astrophysical Journal Supplement Series
- Vol. 215 (2)
- https://doi.org/10.1088/0067-0049/215/2/20
Abstract
No abstract availableThis publication has 50 references indexed in Scilit:
- EINSTEIN A COEFFICIENTS AND OSCILLATOR STRENGTHS FOR THE A 2 Π- X 2 Σ + (RED) AND B 2 Σ + -X 2 Σ + (VIOLET) SYSTEMS AND ROVIBRATIONAL TRANSITIONS IN THE X 2 Σ + STATE OF CNThe Astrophysical Journal Supplement Series, 2014
- Line strengths and updated molecular constants for the C2 Swan systemJournal of Quantitative Spectroscopy and Radiative Transfer, 2013
- IMPROVED log( gf ) VALUES OF SELECTED LINES IN Mn I AND Mn II FOR ABUNDANCE DETERMINATIONS IN FGK DWARFS AND GIANTSThe Astrophysical Journal Supplement Series, 2011
- First stars XII. Abundances in extremely metal-poor turnoff stars, and comparison with the giantsAstronomy & Astrophysics, 2009
- New Light on Stellar Abundance Analyses: Departures from LTE and HomogeneityAnnual Review of Astronomy and Astrophysics, 2005
- The Hamburg/ESO R-process enhanced star survey (HERES)Astronomy & Astrophysics, 2005
- First stars V - Abundance patterns from C to Zn and supernova yields in the early GalaxyAstronomy & Astrophysics, 2004
- The Chemical Composition and Age of the Metal‐poor Halo Star BD +17o3248The Astrophysical Journal, 2002
- Argon branching ratios for spectral intensity calibration: a replyJournal of the Optical Society of America, 1982
- Argon branching ratios for spectral-intensity calibrationJournal of the Optical Society of America, 1981