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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

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