Hostname: page-component-745bb68f8f-kw2vx Total loading time: 0 Render date: 2025-01-13T00:22:24.381Z Has data issue: false hasContentIssue false
  • English
  • Français

An Explanation of the Radio Flux Mystery of HD 192163 and Empirical Models for WN Stars

Published online by Cambridge University Press:  14 August 2015

T. Nugis
T. Nugis*
Affiliation:
W. Struve Astrophysical Observatory of Tartu, Estonia, USSR

Extract

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.

The radio flux value of the star HD 192163 (WN6) measured by Dickel et al. (1980) imposes strong restrictions on the possible mass outflow region models of this star.

Type
SESSION 2 — THE CHEMISTRY OF THE WOLF-RAYET STARS
Information
Symposium - International Astronomical Union , Volume 99: Wolf-Rayet Stars: Observations, Physics, Evolution , 1982 , pp. 127 - 130
Copyright
Copyright © Reidel 1982 

References

Barlow, M.J., Smith, L.J. and Willis, A.J.: 1980, Preprint.Google Scholar
Dickel, H.R., Habing, J.H. and Isaacman, R.: 1980, Ap. J. Lett. 238, L39.CrossRefGoogle Scholar
Holm, A.V. and Cassinelli, J.P.: 1977, Ap. J. 211, 432.CrossRefGoogle Scholar
van der Hucht, K.A., Cassinelli, J.P., Wesselius, P.R. and Wu, Chi-Chao: 1979, Astron. Astrophys. Suppl. 38, 279.Google Scholar
Nugis, T.: 1981, ENSV TA Preprint A-5 (Paper I).Google Scholar