Modelling of Red Giant Stars: The state-of-the-art

被引：9
|
作者：
Cassisi, Santi [1 ]
机构：
[1] INAF Astron Observ Teramo, Via M Maggini Sn, I-64100 Teramo, Italy
来源：
SEISMOLOGY OF THE SUN AND THE DISTANT STARS 2016-USING TODAY'S SUCCESSES TO PREPARE THE FUTURE | 2017年 / 160卷
关键词：
3D CONVECTION SIMULATIONS; STELLAR STRUCTURE MODELS; LUMINOSITY; IMPROVEMENTS; EVOLUTION; ISOCHRONES; CLUSTERS; TRACKS; BUMP; OLD;
D O I：
10.1051/epjconf/201716004002
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The seismic data obtained by the CoRoT and Kepler space missions have provided inferences of the global and structural properties of thousands of red giants. When compared with stellar model predictions, these inferences can significantly improve our understanding of stellar evolution. We present a brief review of the structure and evolution of red giant stars, devoting some emphasis on the major, still open problems.
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页数：13
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