EPJ Web Conf.
Volume 227, 202010th European Summer School on Experimental Nuclear Astrophysics
|Number of page(s)||13|
|Section||Session 1: Lectures|
|Published online||14 January 2020|
Stellar evolution and the Standard Solar Model
1 Physics Department, Pisa University, Largo B. Pontecorvo n.3, I-56127 Pisa
2 INFN, Sezione di Pisa, Largo B. Pontecorvo n.3, I-56127 Pisa
* e–mail: firstname.lastname@example.org
Published online: 14 January 2020
This contribution is meant as a very brief introduction to the principal concepts of stellar physics. First the main physical processes active in stellar structures will be shortly described, then the most important features during the stellar life-cycle up to the central H exhaustion will be summarized with partic-ular attention to the description of solar models.
© The Authors, published by EDP Sciences, 2020
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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