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Li in Chromospherically Active Stars with Large Velocity Components

Published online by Cambridge University Press:  25 May 2016

H. J. Rocha-Pinto ,
B. V. Castilho  and
W. J. Maciel
H. J. Rocha-Pinto
Affiliation:
Depto. de Astronomia, Instituto Astronômico e Geofísico, Universidade de São Paulo, CP 3386, 01060-970, São Paulo SP, Brazil
B. V. Castilho
Affiliation:
Depto. de Astronomia, Instituto Astronômico e Geofísico, Universidade de São Paulo, CP 3386, 01060-970, São Paulo SP, Brazil
W. J. Maciel
Affiliation:
Depto. de Astronomia, Instituto Astronômico e Geofísico, Universidade de São Paulo, CP 3386, 01060-970, São Paulo SP, Brazil

Extract

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We present lithium abundances for nine chromospherically young, kinematically old late-type stars. The data support the interpretation that these objects can be formed during the coalescence of a short-period binary.

Type
6. Stellar Knowledge to and from Light Elements
Information
Symposium - International Astronomical Union , Volume 198: The Light Elements and their Evolution , 2000 , pp. 512 - 513
Copyright
Copyright © Astronomical Society of the Pacific 2000 

References

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