No CrossRef data available.
Article contents
Wind characteristics of the 07 n star HD 217086 in the Cep OB 3 association
Published online by Cambridge University Press: 12 April 2016
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.
The 07 n star HD 217086 which provides the ionization of the H II region S 155 A and is the brightest member of the Cep OB 3 association, has been observed in the ultraviolet with IUE. From an analysis of the UV spectra we determine a terminal velocity of 3560 ± 100 km s-1 and a mass loss rate of . A comparison is made with the stars of similar spectral type.
- Type
- Session I - Winds from Early Type Stars: Observations
- Information
- International Astronomical Union Colloquium , Volume 59: Effects of Mass Loss on Stellar Evolution , 1981 , pp. 41 - 44
- Copyright
- Copyright © Reidel 1981
References
Abbott, D.C., Bieging, J.H., Churchwell, E.D., and Cassinelli, J.P.: 1980, Astrophys. J. .238, pp. 196–202.Google Scholar
Beichman, C.A., Becklin, E.E., Wynn-Williams, S.G.: 1979, Astrophys. J. (Letters) 232, L47–L51.Google Scholar
Felli, M., Tofani, G., Harten, R.H., and Panagia, N.: 1978, Astron. Astrophys.
69, pp. 199–211.Google Scholar