Broadening of lines of Be II, Sr II and Ba II by collisions with hydrogen atoms and the solar abundance of strontium
Open Access
- 21 January 2000
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 311 (3) , 535-540
- https://doi.org/10.1046/j.1365-8711.2000.03090.x
Abstract
No abstract availableKeywords
This publication has 19 references indexed in Scilit:
- The broadening of strong lines of Ca+, Mg+ and Ba+ by collisions with neutral hydrogen atomsMonthly Notices of the Royal Astronomical Society, 1998
- The broadening of d–f and f–d transitions by collisions with neutral hydrogen atomsMonthly Notices of the Royal Astronomical Society, 1998
- Shallow mixing in the solar photosphere inferred from revised beryllium abundancesNature, 1998
- Standard Solar CompositionSpace Science Reviews, 1998
- The broadening of p-d and d-p transitions by collisions with neutral hydrogen atomsMonthly Notices of the Royal Astronomical Society, 1997
- Width cross-sections for collisional broadening of s–p and p–s transitions by atomic hydrogenMonthly Notices of the Royal Astronomical Society, 1995
- An investigation of Brueckner's theory of line broadening with application to the sodium D linesMonthly Notices of the Royal Astronomical Society, 1991
- First detection of beryllium in a very metal poor star - A test of the standard big bang modelThe Astrophysical Journal, 1991
- Solar abundances of lithium, beryllium and boronSolar Physics, 1968
- Oscillator Strengths of Ca II, Sr II, and Ba IIPhysical Review B, 1967