S-type Stars: LaO Line List for the B2Σ+-X2Σ+ Band System

被引:3
|
作者
Bernath, P. F. [1 ,2 ]
Dodangodage, R. [2 ]
Lievin, J. [3 ]
机构
[1] Old Dominion Univ, Dept Chem & Biochem, Norfolk, VA 23529 USA
[2] Old Dominion Univ, Dept Phys, Norfolk, VA 23529 USA
[3] Univ Libre Bruxelles, Spect Quantum Chem & Atmospher Remote Sensing, CP 160 09 Av F D Roosevelt 50, Brussels, Belgium
来源
ASTROPHYSICAL JOURNAL | 2022年 / 933卷 / 01期
关键词
ELECTRIC-DIPOLE MOMENTS; RADIATIVE LIFETIMES; HYPERFINE-STRUCTURE; LANTHANUM MONOXIDE; COMPUTER-PROGRAM; BASIS-SETS; LASER; SPECTROSCOPY; STATES; TRANSITION;
D O I
10.3847/1538-4357/ac731f
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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 B-2 Sigma(+)-X-2 Sigma(+) and A(2)Pi-X-2 Sigma(+) band systems can be used to determine the La abundances in cool S stars. The bands of the B-2 Sigma(+)-X-2 Sigma(+) 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 B-2 Sigma(+)-X-2 Sigma(+) band system that can be used to determine La abundances.
引用
收藏
页数:7
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