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Oxygen Abundances from Infrared OH Lines

Published online by Cambridge University Press:  30 March 2016

Suchitra C. Balachandran ,
John S. Carr  and
Bruce W. Carney
Suchitra C. Balachandran
Affiliation:
Department of Astronomy, University of Maryland, College Park MD 20740, USA
John S. Carr
Affiliation:
Naval Research Laboratory, 4555 Overlook Avenue, Washington, DC 20375
Bruce W. Carney
Affiliation:
Department of Physics and Astronomy, University of North Carolina, Chapel Hill NC 27599, USA

Abstract

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Oxygen abundances are derived from IR-OH lines and compared to published results from UV-OH lines.

Type
II. Joint Discussions
Information
Highlights of Astronomy , Volume 12: Highlights of Astronomy. As presented at the XXIVth General Assembly of the IAU, 2000 , 2002 , pp. 420 - 422
Copyright
Copyright © Astronomical Society of Pacific 2002

References

Alonso, A., Arribas, S., & Martínez-Roger, C. 1999, A&AS, 140, 261 Google Scholar
Balachandran, S.C., & Carney, B.W. 1996, AJ, 111, 946 Google Scholar
Boesgaard, A.M., King, J.R., Deliyannis, C.P., & Vogt, S.S. 1999, AJ, 118, 2542 Google Scholar
Grevesse, N., Sauval, A.J., & van Dischoeck, E.F. 1984, A&A, 141, 10 Google Scholar
Israelian, G., García López, R.J., & Rebolo, R. 1998, ApJ, 507, 805 Google Scholar
Kiselman, D. 1991, A&A, 235, L9 Google Scholar
Meléndez, J., Barbuy, B., & Spite, F. 2001, ApJ, 556, 858 Google Scholar