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High Resolution Interferometry of Cool Stars

Published online by Cambridge University Press:  30 March 2016

D. L. Lambert
D. L. Lambert*
Affiliation:
McDonald Observatory and Dept. of Astronomy, The University of Texas at Austin, Austin, Tex., U.S.A.

Abstract

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This paper reviews results obtained in a program of high resolution infrared spectroscopy of K and M giants. The reported results include (i) a preliminary analysis of the C, N and O abundances for α Ori, (ii) determinations of the 12C/13C and 16O/18O ratios for α Ori (12C/13C ~ 6 and 16O/18 ~ 500), (iii) the derivation of a lower limit, 16O/18O≳ 300, for the 160/18O ratio in α Boo, (iv) a discussion of observations of the SiO first-overtone vibration-rotation bands in M stars, and (v) a search for the fundamental quadrupole vibration-rotation lines of H2.

Type
Joint Discussions
Information
Highlights of Astronomy , Volume 3: Highlights of Astronomy. As presented at the XVth General Assembly of the IAU, 1973 , 1974 , pp. 237 - 254
Copyright
Copyright © Reidel 1974

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