Hostname: page-component-586b7cd67f-t7fkt Total loading time: 0 Render date: 2024-11-26T20:41:01.874Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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