Document Type
Article
Publication Date
2022
DOI
10.3847/1538-4357/ac731f
Publication Title
The Astrophysical Journal
Volume
933
Issue
1
Pages
99 (1-7)
Abstract
LaO bands are a characteristic feature in the spectrum of cool S-type stars. La is made primarily by the s-process during the asymptotic giant branch phase of stellar evolution. The B2Σ+–X2Σ+ and A2Π–X2Σ+ band systems can be used to determine the La abundances in cool S stars. The bands of the B2Σ+–X2Σ+ with v' and v" ⩽ 5 have been rotationally analyzed from an emission spectrum from a carbon furnace. Line strengths are calculated using an ab initio transition dipole function, corrected using experimental lifetimes. We provide a line list for the B2Σ+–X2Σ+ band system that can be used to determine La abundances.
Original Publication Citation
Bernath, P.F., Dodangodage, R., Liévin, J. (2022) S-type stars: LaO line list for the B²Σ⁺-X²Σ⁺ band system. The Astrophysical Journal, 933 (1) 1-7, Article 99. https://doi.org/10.3847/1538-4357/ac731f
ORCID
0000-0002-1255-396X (Bernath), 0000-0003-4814-4970 (Dodangodage)
Repository Citation
Bernath, P. F.; Dodangodage, Randika; and Liévin, J., "S-Type Stars: LaO Line List for the B²Σ⁺-X²Σ⁺ Band System" (2022). Chemistry & Biochemistry Faculty Publications. 227.
https://digitalcommons.odu.edu/chemistry_fac_pubs/227
Included in
Inorganic Chemistry Commons, Physical Chemistry Commons, Stars, Interstellar Medium and the Galaxy Commons
Comments
© 2022 The Authors.
Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 Licence.