Year: 2013
Type: conference-paper
Abstract: In spite of the great effort made in the last decades to improve our understanding of stellar evolution, significant uncertainties still remain due to our poor knowledge of some complex physical processes that still require an empirical calibration, such as the efficiency of convective heat transport and interior mixing. Here we will review the impact of these uncertainties on the evolution of red giant stars.
Source: EPJ Web of Conferences
Authors: A. Bressan, P. Marigo, L. Girardi, A. Nanni, S. Rubele
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: diamond
OpenAlex ID: W2163383495
