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Key Issues: A Round Table Discussion

Published online by Cambridge University Press:  12 April 2016

T.M. Brown ,
P. Demarque ,
R. Noyes ,
F. Praderie ,
I.W. Roxburgh  and
E. Schatzman
T.M. Brown
Affiliation:
High Altitude Observatory, National Center of Atmospheric Research. P. 0. Box 3000. Boulder, CO 80307, USA
P. Demarque
Affiliation:
Yale University, Department of Astronomy, P.O. Box 6606, New Haven, CT 06511, USA
R. Noyes
Affiliation:
Smithonian Astrophysical Observatory, 60 Garden Street, Cambridge, MA 02138, USA
F. Praderie
Affiliation:
DESPA, URA CNRS 264, Observatoire de Paris, 92195 Meudon Cedex, France
I.W. Roxburgh
Affiliation:
School of Mathematical Science, Queen Mary College, Mile End Road, London, E14NS, UK
E. Schatzman
Affiliation:
DASGAL. URA CNRS 335, Observatoire de Paris, 92195 Meudon Cedex, France

Extract

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We have taken part to an exceptionally rich colloquium, characterized by a large amount of information in all fields of physics, and a remarkable collection of observational data. Our understanding of what is going on inside the stars has changed in a radical manner during the last years, on one side because the observations are bringing new kinds of information, and on the other side because theory in its development is taking into account a number of processes, some of them having been completely ignored only ten years ago.

It is impossible to draw here a complete list of problems. There are many cases where some inconsistency could be found in the theory itself or some contradiction between observational data and theory. I recommended that such a list should be drawn carefully. The participants to the round table discussion will give their contribution, helping to open the way to new fields of research and to new discoveries.

Type
X. Round Table
Information
International Astronomical Union Colloquium , Volume 137: Inside the Stars , 1993 , pp. 776 - 786
Copyright
Copyright © Astronomical Society of the Pacific 1993

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