Hostname: page-component-6bf8c574d5-r8w4l Total loading time: 0 Render date: 2025-03-09T16:26:14.556Z Has data issue: false hasContentIssue false
  • English
  • Français

Light Elements as Probes of Stellar Interiors

Published online by Cambridge University Press:  19 July 2016

A. Baglin  and
P.-J. Morel
A. Baglin
Affiliation:
Observatoire de Nice, B.P. n° 139, 06003 NICE Cedex, France
P.-J. Morel
Affiliation:
Observatoire de Nice, B.P. n° 139, 06003 NICE Cedex, France

Extract

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.

For stars cooler than 6400°K, the lithium is observed to be depleted with respect to the universal value for Population I stars. The depletion depends on mass and age and occurs, both during the main-sequence (Hyades) and the pre-main-sequence (Pleiades).

Type
IV. Spectroscopic Patterns of Stellar Atmospheres
Information
Symposium - International Astronomical Union , Volume 132: The Impact of Veryhigh S/N Spectroscopy on Stellar Physics , 1988 , pp. 279 - 282
Copyright
Copyright © Kluwer 1988 

References

Baglin, A., Morel, P.-J., Schatzman, E.: 1985, Astron. Astrophys. 149, 309.Google Scholar
Cayrel, R., Cayrel de Strobel, G., Campbell, B., Däppen, W.: 1984, Astrophys. J. 283, 205.CrossRefGoogle Scholar
Christensen-Dalsgaard, J., Duvall, T.L. Jr, Gough, D.O., Harvey, J.W., Rhodes, E.J. Jr: 1985, Nature 315, 378.CrossRefGoogle Scholar
Demarque, P., Guenter, D.B., van Altena, W.F.: 1986, Astrophys. J. 300, 773.Google Scholar
Lebreton, Y., Maeder, A.: 1986, Astron. Astrophys. 161, 119.Google Scholar
Schatzman, E.: 1977, Astron. Astrophys. 56, 211.Google Scholar
Zahn, J.-P.: 1984, in “Instabilités hydrodynamiques et applications astrophysiques”, p. 389, eds. Baglin, A. et Auvergne, M., S.F.S.A. Paris.Google Scholar