Hostname: page-component-84b7d79bbc-rnpqb Total loading time: 0 Render date: 2024-07-30T05:21:19.286Z Has data issue: false hasContentIssue false
  • English
  • Français

Round Table Summary: Winds and Pulsating Stars

Published online by Cambridge University Press:  26 May 2016

Lee Anne Willson
Lee Anne Willson*
Affiliation:
Department of Physics and Astronomy, Iowa State University, Ames IA 50011, USA

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.

Speakers for this session were selected according to our perceptions about the frontier areas in dynamical atmospheres, the atmospheres of very cool stars, and stellar winds. This summary of posters and topics raised in the round table discussion opens with a brief summary of current issues in modeling pulsating stars and winds. Observational constraints are emphasized in Section 3. on “peeling the onion” of the atmosphere/wind structure. Section 4. covers a variety of methods for detecting and measuring stellar winds. The concluding remarks include some questions facing theorists and observers working in this field.

Type
Session F. Winds - Cool and Pulsating Stars
Information
Symposium - International Astronomical Union , Volume 210: Modelling of Stellar Atmospheres , 2003 , pp. 403 - 411
Copyright
Copyright © Astronomical Society of the Pacific 2003 

References

Bowen, G. H. 1988, ApJ, 329, 299 Google Scholar
Bowen, G. H., Willson, L. A. 1991, ApJ, 375, L53 Google Scholar
Hill, S. J., Willson, L. A. 1979, ApJ, 229, 1029 Google Scholar
Kudritzki, R., Puls, J. 2000, ARA&A, 38, 613 Google Scholar
Olofsson, H., Carlstrom, U., Eriksson, K., Gustafsson, B., Willson, L. A. 1990, A&A, 230, L13 Google Scholar
Willson, L. A., Wallerstein, G., Pilachowski, C. A. 1982, MNRAS, 198, 483 CrossRefGoogle Scholar
Willson, L. A. 2000, ARA&A, 38, 573 Google Scholar