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Theoretical evidence of mass loss from globular cluster stars
Published online by Cambridge University Press: 12 April 2016
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