Rotation, Activity and Lithium Depletion in the Hyades Late Main Sequence

Bibcode
1988IAUS..132..469R
Rebolo, R.; Beckman, J. E.
Referencia bibliográfica

The Impact of Very High S/N Spectroscopy on Stellar Physics: Proceedings of the 132nd Symposium of the International Astronomical Union held in Paris, France, June 29-July 3, 1987. Edited by G. Cayrel de Strobel and Monique Spite. International Astronomical Union. Symposium no. 132, Kluwer Academic Publishers, Dordrecht., p.469

Fecha de publicación:
0
1988
Número de autores
2
Número de autores del IAC
0
Número de citas
1
Número de citas referidas
1
Descripción
Selecting stars with previously measured or estimated rotational periods the authors measured Li equivalent widths in 8 stars of the Hyades late main sequence. Plotting log N(Li) against Rossby number the authors can separate the effects of temperature and rotation. They find for stars later than F8 increased depletion with longer period, at constant surface temperature. The authors give a tentative view of the implications of these results for stellar modelling.
Tipo
Sin árbitro

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