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The nature of V Sagittae

Published online by Cambridge University Press:  12 April 2016

Janet H. Wood
Affiliation:
Department of Physics, Keele University, Keele, ST5 5BG, UK
J.J. Lockley
Affiliation:
Department of Physics, Keele University, Keele, ST5 5BG, UK

Abstract

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We discuss previous models of V Sge and, in light of our new phase resolved spectroscopy data, suggest a new model: a colliding wind.

Type
Part 10. Accretion Disks and Outflows
Copyright
Copyright © Astronomical Society of the Pacific 1997

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