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The nature of V Sagittae

Published online by Cambridge University Press:  12 April 2016

Janet H. Wood  and
J.J. Lockley
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
Information
International Astronomical Union Colloquium , Volume 163: Accretion Phenomena and Related Outflows , 1997 , pp. 457 - 460
Copyright
Copyright © Astronomical Society of the Pacific 1997

References

Herbig, G.H., Preston, G.W., Smak, J., Paczyński, B., 1965, Ap.J., 141, 617 CrossRefGoogle Scholar
Koch, R.H., Corcoran, M.F., Holenstein, B.D., McClusky, G.E., 1986, Ap.J., 306, 618 Google Scholar
Lockley, J.J., Wood, J.H., Eggleton, P.P., 1996, in preparation.Google Scholar
Lockley, J.J., Wood, J.H., Shugarov, S., Naylor, T., Catalan, M.S., 1996, to be submitted to MNRAS.Google Scholar
Lührs, S., 1995, in “Wolf-Rayet Stars, Binaries, Colliding Winds and Evolution”, eds. van der Hucht, K.A., Williams, P.M., p 416 Google Scholar
Mader, J., 1996, MSc thesis, San Diego State University.Google Scholar
Ritter, H., 1990, A&AS, 85, 1179.Google Scholar
Wallerstein, G., Willson, L.A., Salzer, J., Brugel, E., 1984, A&A, 133, 137 Google Scholar
Williams, G., King, A.R., Uomoto, A.K., Hiltner, W.A., 1983, MNRAS, 219, 809 CrossRefGoogle Scholar