The photospheric barium spectrum: Solar abundance and collision broadening of Baii lines by hydrogen
- 1 November 1974
- journal article
- research article
- Published by Springer Nature in Solar Physics
- Vol. 39 (1) , 19-30
- https://doi.org/10.1007/bf00154968
Abstract
No abstract availableKeywords
This publication has 21 references indexed in Scilit:
- The solar abundance of calcium and collision broadening of Ca i- and Ca ii-Fraunhofer lines by hydrogenSolar Physics, 1972
- Collision Broadening by Neutral HydrogenThe Astrophysical Journal, 1971
- Meteorites and the Early Solar SystemAnnual Review of Astronomy and Astrophysics, 1971
- The Harvard-Smithsonian reference atmosphereSolar Physics, 1971
- Broadening of the SodiumLines by Atomic Hydrogen. An Analysis in Terms of the NaH Molecular PotentialsPhysical Review A, 1971
- The Abundances of the Elements in the Solar Photosphere--V: The Alkaline Earths Mg, Ca, Sr, BaMonthly Notices of the Royal Astronomical Society, 1968
- The Chromospheric Spectrum at the 1962 EclipseThe Astrophysical Journal Supplement Series, 1968
- Oscillator Strengths of Ca II, Sr II, and Ba IIPhysical Review B, 1967
- Faint Lines in the Arc Spectrum of Iron (Fe I).Journal of Research of the National Bureau of Standards Section A: Physics and Chemistry, 1961
- The Abundances of the Elements in the Solar Atmosphere.The Astrophysical Journal Supplement Series, 1960