arXiv Analytics

Sign in

arXiv:1409.2281 [astro-ph.SR]AbstractReferencesReviewsResources

Uncertainties in models of stellar structure and evolution

Arlette Noels, Angela Bragaglia

Published 2014-09-08Version 1

Numerous physical aspects of stellar physics have been presented in Ses- sion 2 and the underlying uncertainties have been tentatively assessed. We try here to highlight some specific points raised after the talks and during the general discus- sion at the end of the session and eventually at the end of the workshop. A table of model uncertainties is then drawn with the help of the participants in order to give the state of the art in stellar modeling uncertainties as of July 2013.

Comments: Proc. of the workshop "Asteroseismology of stellar populations in the Milky Way" (Sesto, 22-26 July 2013), Astrophysics and Space Science Proceedings, (eds. A. Miglio, L. Girardi, P. Eggenberger, J. Montalban)
Categories: astro-ph.SR
Related articles: Most relevant | Search more
arXiv:1007.1720 [astro-ph.SR] (Published 2010-07-10)
Seismological challenges for stellar structure
arXiv:1606.09448 [astro-ph.SR] (Published 2016-06-30)
Clusters: age scales for stellar physics
arXiv:1907.10315 [astro-ph.SR] (Published 2019-07-24)
Revisiting Kepler-444 Part I. Seismic modelling and inversions of stellar structure
G. Buldgen et al.