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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

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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

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