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Hipparcos and Theory of Stellar Interiors

Published online by Cambridge University Press:  14 August 2015

A. Baglin
A. Baglin*
Affiliation:
DESPA, Observatoire de Paris, URA CNRS 264, 5 place J. Janssen, Meudon CEDEX, France.

Extract

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The theory of stellar interiors is generally considered as well settled, and many branches of astrophysics rely on its results. However, the true situation is not so bright. Despite great successes at its beginning, in the sixties, it has to deal with many physical processes, generally poorly understood, which have large influences on the results and the derived quantities, like for instance ages.

After a rapid description of these difficulties, I will recall the majorquestions of the confrontation between theory and observations, and how HIPPARCOS can and will help. As an illustration, a few preliminary results will be presented, and future prospects foreseen. But, this short review is byno means exhaustive; there are many more results dealing directly or indirectly with stellar structure theory which have already been presented at theVenice Symposium (Perryman et al, 1997a), and many more, I am not aware of, will certainly appear soon.

Type
II. Joint Discussions
Information
Highlights of Astronomy , Volume 11 , Issue 1: Highlights of Astronomy. As presented at the XXIIIrd General Assembly of the IAU (Part A), 1997 , 1998 , pp. 555 - 557
Copyright
Copyright © Kluwer 1998

References

Baglin, A.(1987) in Scientific aspects of the Input Catalogue Preparation II, Torra, J. and Turon, C. eds, p. 103.Google Scholar
Canuto, V.M., Goldman, I., Mazitelli, I.(1996) Astrophys. J., 473, 550.Google Scholar
Cayrel, R., Lebreton, Y., Perrin, M.N., Turon, C. (1997), Hipparcos symposium Venice, ESA publ. SP-402, p. 219.Google Scholar
Fernandes, J. (1997) Ph. D. Thesis, Paris VII University Google Scholar
Fernandes, J., Lebreton, Y., Baglin, A. (1997), Astron. Astrophys, in press.Google Scholar
Høg, E., Petersen, J.O.(1997), Astron. Astrophys., in press.Google Scholar
Lebreton, Y., Michel, E., Goupil, M.J., Baglin, A., Fernandes, J. (1994), IAU Symposium 166, p.135.Google Scholar
Lebreton, Y., Baglin, A.(1995) in Stellar evolution, what should be done? 32th Liege Inst. Astroph. Coll, p.1.Google Scholar
Lebreton, Y., Perrin, M.N., Fernandes, J. et al. (1997) Hipparcos symposium Venice, ESA publ. SP-402, p. 379.Google Scholar
Liu, Y. Y, Baglin, A., Auvergne, M. et al. (1997) Hipparcos symposium Venice, ESA publ. SP-402, p. 363.Google Scholar
Martin, C, Mignard, F. (1997), Astron. Astrophys, in pressGoogle Scholar
Mermilliod, J.C., Turon, C., Robichon, N. et al. (1997), Hipparcos symposium Venice, ESA publ. SP-402, p. 643.Google Scholar
Noels, A., Grevesse, N., Magain, P., Neuforge, C., Baglin, A., Lebreton, Y. (1991), Astron, Astrophys, 247, 91.Google Scholar
North, P., Jaschek, C., Egret, D. (1997)Hipparcos symposium Venice, ESA publ. SP-402, p. 367.Google Scholar
Perryman, M.A.C., et al. (1997a), Hipparcos symposium Venice, ESA publ. SP-402,Google Scholar
Perryman, M.A.C., Brown, A.G.A., Lebreton, Y. et al. (1997b), Astron. Astrophys., in press.Google Scholar
Pont, F., Charbonnel, C., Lebreton, Y. et al. (1997), Hipparcos symposium Venice, ESA publ. SP-402, p. 699.Google Scholar
Robichon, N., Arenou, F., Turon, C., et al. (1997), Highlights in Astronomy, 11, in press.Google Scholar
Roxburgh, I.W., (1997) IAU symposium 185, in press.Google Scholar
Schatzman, E..(1995) in Stellar evolution, what should be done? 32th Liege Inst. Astroph. Coll, p.121.Google Scholar
Soderhjelm, S., Lindengren, L., Perryman, M.A.C. (1997), Hipparcos symposium Venice, ESA publ. SP-402, p.251.Google Scholar
Zahn, J.P.(1995) in Stellar evolution, what should be done? 32th Liege Inst. Astroph. Coll, p.111.Google Scholar