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A New Absorption-Line Orbit for the Symbiotic Nova AG Pegasi

Published online by Cambridge University Press:  12 April 2016

M.H. Slovak  and
D.L. Lambert
M.H. Slovak
Affiliation:
University of Wisconsin, Madison, Wisconsin, USA
D.L. Lambert
Affiliation:
University of Texas, Austin, Texas, USA

Abstract

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Precise cross-correlation absorption-line velocities have been derived using high resolution near infrared coude’ spectra for the symbiotic nova AG Pegasi. A revised weighted orbital solution is presented based on both extant photographic and the new absorption-line velocities.

Type
Session 3. Physics of Individual Objects
Information
International Astronomical Union Colloquium , Volume 103: The Symbiotic Phenomenon , 1988 , pp. 265 - 267
Copyright
Copyright © Kluwer 1988

References

Cowley, A., and Stencel, R. 1973, Ap. J. 184, 687.CrossRefGoogle Scholar
Fernie, J.D. 1987, Pub. A. S. P., 97, 653.Google Scholar
Hutchings, J.B., Cowley, A.P., and Redman, R.O. 1975, Ap. J., 201, 404.Google Scholar
Merrill, P.W. 1951, Ap. J., 113, 605.Google Scholar
Merrill, P.W. 1959, ibid, 129, 44.Google Scholar
Slovak, M.H. 1982, PhD Thesis (University of Texas: Austin).Google Scholar
Vogt, S.S., Tuli, R.G., and Kelton, P.W. 1987, Applied Optics, 17, 574.Google Scholar
Wilson, R.E. 1953, General Catalogue of Stellar Radial Velocities (Washington: Carnegie), Publication 601.Google Scholar