S-type Stars: LaO Line List for the B 2 Σ + –X 2 Σ + Band System
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 Σ + –X 2 Σ + and A 2 Π–X 2 Σ + band systems can be used to determine the La abundances in cool S stars. The bands...
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Veröffentlicht in: | The Astrophysical journal 2022-07, Vol.933 (1), p.99 |
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Hauptverfasser: | , , |
Format: | Artikel |
Sprache: | eng |
Online-Zugang: | Volltext |
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Zusammenfassung: | 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
Σ
+
–X
2
Σ
+
and A
2
Π–X
2
Σ
+
band systems can be used to determine the La abundances in cool S stars. The bands of the B
2
Σ
+
–X
2
Σ
+
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
Σ
+
–X
2
Σ
+
band system that can be used to determine La abundances. |
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ISSN: | 0004-637X 1538-4357 |
DOI: | 10.3847/1538-4357/ac731f |