S-type Stars: LaO Line List for the B2Σ+-X2Σ+ Band System
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作者:
Bernath, P. F.
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Old Dominion Univ, Dept Chem & Biochem, Norfolk, VA 23529 USA
Old Dominion Univ, Dept Phys, Norfolk, VA 23529 USAOld Dominion Univ, Dept Chem & Biochem, Norfolk, VA 23529 USA
Bernath, P. F.
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Dodangodage, R.
[2
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Lievin, J.
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Univ Libre Bruxelles, Spect Quantum Chem & Atmospher Remote Sensing, CP 160 09 Av F D Roosevelt 50, Brussels, BelgiumOld Dominion Univ, Dept Chem & Biochem, Norfolk, VA 23529 USA
Lievin, J.
[3
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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
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.