Hostname: page-component-cb9f654ff-9knnw Total loading time: 0 Render date: 2025-09-02T09:11:21.212Z Has data issue: false hasContentIssue false
  • English
  • Français

Introductory overview

Published online by Cambridge University Press:  25 May 2016

J. Andersen
J. Andersen*
Affiliation:
Astronomical Observatory; Niels Bohr Institute for Astronomy, Physics, and Geophysics; Juliane Maries Vej 30, DK-2100 Copenhagen, Denmark

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 subject of this meeting is the confrontation between precise observational and theoretical determinations of fundamental stellar properties. Its goal is to better define the limits of our present understanding of the structure and evolution of stars, and of our own and other galaxies. That goal is not approached by keeping to the “safe” side of the border: The areas where significant disagreement is found between the best observations and the best theories also show the directions where progress is to be made.

References

Barbuy, B., Cayrel, R., Spite, M., Beers, T.C., Spite, F., Nordstrom, B., Nissen, P.E. 1997, A&A 317, L63 Google Scholar
Edvardsson, B., Andersen, J., Gustafsson, B., Lambert, D.L., Nissen, P.E., Tomkin, J. 1993, A&A 275, 101 Google Scholar
Nissen, P.E., Schuster, W.J. 1997, A&A, in press Google Scholar
Nordström, B. 1989, ApJ, 341, 934 Google Scholar
Nordström, B., Andersen, J., Andersen, M.I. 1997, this meeting; poster paper no. 64 Google Scholar
Popper, D.M. 1970, in Mass Loss and Evolution in Close Binaries, (IAU Colloquium No. 6), eds. Gyldenkerne, K. and West, R.M., Univ. of Copenhagen, Copenhagen, p. 13 Google Scholar
Popper, D.M. 1973, ApJ 185, 265 Google Scholar
Refsdal, S., Roth, M.L., Weigert, A. 1974, A&A 36, 113 Google Scholar
Sneden, C., McWilliam, A., Preston, G.W., Cowan, J.J., Burris, D., Armosky, B.J. 1996, ApJ 467, 819 CrossRefGoogle Scholar