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Grain sedimentation and main sequence evolution

Published online by Cambridge University Press:  04 August 2017

John Lattanzio
John Lattanzio*
Affiliation:
Department of Mathematics, Monash University, Clayton, Victoria, Australia

Abstract

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Under the assumption that grain sedimentationcan lead to an enhancement of heavy elements in the central regions of proto-stars, we present the evolution of stellar models with metal-rich cores. The resulting isochrones can explain the “double-gap” clusters NGC2420 and NGC2506, without destroying the agreement for other clusters.

Information

Type
I. EVOLUTION OF LOW AND INTERMEDIATE MASS STARS OBSERVATIONS AND MODELS
Information
Symposium - International Astronomical Union , Volume 105: Observational Tests of the Stellar Evolution Theory , 1984, pp. 109 - 112
Copyright
Copyright © Reidel 1984 

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