Carbon and Oxygen Isotopic Ratios. II. Semiregular Variable M Giants

Carbon and oxygen isotopic ratios are reported for a sample of 51 SRb- and Lb-type variable asymptotic giant branch stars. Vibration-rotation first- and second-overtone CO lines in 1.5-2.5 m spectra were measured to derive isotopic ratios for 12C/13C, 16O/17O, and 16O/18O. Comparisons with previous...

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Veröffentlicht in:The Astrophysical journal 2019-12, Vol.886 (2), p.117
Hauptverfasser: Lebzelter, Thomas, Hinkle, Kenneth H., Straniero, Oscar, Lambert, David L., Pilachowski, Catherine A., Nault, Kristie A.
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container_issue 2
container_start_page 117
container_title The Astrophysical journal
container_volume 886
creator Lebzelter, Thomas
Hinkle, Kenneth H.
Straniero, Oscar
Lambert, David L.
Pilachowski, Catherine A.
Nault, Kristie A.
description Carbon and oxygen isotopic ratios are reported for a sample of 51 SRb- and Lb-type variable asymptotic giant branch stars. Vibration-rotation first- and second-overtone CO lines in 1.5-2.5 m spectra were measured to derive isotopic ratios for 12C/13C, 16O/17O, and 16O/18O. Comparisons with previous measurements for individual stars and with various samples of evolved stars, as available in the extant literature, are discussed. Using the oxygen isotopic ratios, the masses of the SRb stars can be derived. Combining the masses with Gaia luminosities, the SRb stars are shown to be antecedents of the Mira variables. The limiting parameters where plane-parallel, hydrostatic equilibrium model atmospheres can be used for abundance analysis of M giants are explored.
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subjects Astrophysics
Asymptotic giant branch stars
Carbon
High resolution spectroscopy
Isotopes
Isotopic abundances
Late stellar evolution
Long period variable stars
Mira variables
Oxygen
Semi-regular variable stars
Stellar evolution
Stellar nucleosynthesis
Stellar rotation
Vibration
title Carbon and Oxygen Isotopic Ratios. II. Semiregular Variable M Giants
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