Hostname: page-component-745bb68f8f-l4dxg Total loading time: 0 Render date: 2025-01-11T05:08:19.885Z Has data issue: false hasContentIssue false
  • English
  • Français

How are we doing so far? A summary of the Symposium

Published online by Cambridge University Press:  02 March 2005

Michael M. Dworetsky
Michael M. Dworetsky
Affiliation:
Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, UK email: [email protected]
Rights & Permissions [Opens in a new window]

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.

Some highlights of Symposium 224 on “The A-Star Puzzle” are reviewed and transcribed from the author's ad hoc oral presentation on the final day of the meeting. Articles referred to are all contained in this volume, hence there are no figures or references. Topics include theory and observations of normal A stars, HgMn, Am, and Ap stars, $\lambda$ Boo stars, magnetic fields, rotation, convection, pulsations, supergiant stars, and observational methods including polarimetry, spectroscopy, and photometry.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Keywords

Stars: abundancesstars: chemically peculiarstars: horizontal-branchstars: magnetic fieldsstars: pre-main-sequence
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS224 , July 2004 , pp. 499 - 504
Copyright
© 2004 International Astronomical Union