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Theoretical evidence of mass loss from globular cluster stars

Published online by Cambridge University Press:  12 April 2016

V. Castellani  and
A. Tornambè
V. Castellani
Affiliation:
Istituto di Astrofisica Spaziale, Frascati
A. Tornambè
Affiliation:
Istituto di Astrofisica Spaziale, Frascati

Summary

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The total amount of mass lost during the first giant phase of Population II red giants is derived from Horizontal Branch properties: it is found to be proportional to the metal content.

Type
Session VI - Mass Loss and Stellar Evolution: Low Mass Stars
Information
International Astronomical Union Colloquium , Volume 59: Effects of Mass Loss on Stellar Evolution , 1981 , pp. 357 - 359
Copyright
Copyright © Reidel 1981

References

Caputo, F., Di Gregorio, R.: 1980, Internal Report n. 33 of the Istituto di Astrofisica Spaziale.Google Scholar
Castellani, V., Tornambè, A.: 1977, Astron. Astrophys. 61, 427.Google Scholar
Castellani, V., Tornambè, A.: 1980, Astron. Astrophys., in press.Google Scholar
Rood, R.T.: 1980, Private communication.Google Scholar