Hostname: page-component-cd9895bd7-jn8rn Total loading time: 0 Render date: 2024-12-26T03:14:25.053Z Has data issue: false hasContentIssue false
  • English
  • Français

Line profiles in expanding atmospheres

Published online by Cambridge University Press:  26 May 2016

L. Cidale
L. Cidale*
Affiliation:
Observatorio de La Plata - Paseo del Bosque S/N - 1900 La Plata - Argentina

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 analysis of the UV resonance transitions of superionized species observed in early-type stars suggests the presence of a high temperature region and an outward flow of matter (Snow & Marlborough 1976).

Type
7. OB Stellar Winds
Information
Symposium - International Astronomical Union , Volume 162: Pulsation, Rotation and Mass Loss in Early-Type Stars , 1994 , pp. 496 - 497
Copyright
Copyright © Kluwer 1994 

References

Catala, C., and Kunasz, P. B.: 1987, A&A 174, 158 Google Scholar
Cidale, L. S., and Ringuelet, A. E.: 1993, ApJ 411, 874 CrossRefGoogle Scholar
Mihalas, D., and Kunasz, P. B.: 1978, ApJ 219, 635 CrossRefGoogle Scholar
Snow, T. P., and Marlborough, J. M.: 1976, ApJ 203, L87 CrossRefGoogle Scholar