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A critical test to disentangle the role of overshooting and rotation in stars

Published online by Cambridge University Press:  30 December 2019

G. Costa
Affiliation:
SISSA, via Bonomea 365, Trieste, Italy
L. Girardi
Affiliation:
OAPD–INAF, Vicolo dell’Osservatorio 5, Padova, Italy
A. Bressan
Affiliation:
SISSA, via Bonomea 365, Trieste, Italy
P. Marigo
Affiliation:
Dipartimento di Fisica e Astronomia Galileo Galilei, Università di Padova, Italy
Y. Chen
Affiliation:
Dipartimento di Fisica e Astronomia Galileo Galilei, Università di Padova, Italy
B. Kanniah
Affiliation:
MIT, Cambridge, Massachusetts, USA
A. Lanza
Affiliation:
SISSA, via Bonomea 365, Trieste, Italy
T. S. Rodrigues
Affiliation:
OAPD–INAF, Vicolo dell’Osservatorio 5, Padova, Italy
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Abstract

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We study the mixing in low-intermediate massive stars using eclipsing binaries. We compute stellar evolutionary models with a varying convective core overshooting parameter and different rotation rates. Using a Bayesian estimation method, we found that the coexistence of the two phenomena may be a reasonable explanation of the observed extra-mixing.

Type
Contributed Papers
Copyright
© International Astronomical Union 2019 

References

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