The Early Evolution of Solar-type Stars: Star-Disk Interaction and the Photometric Variability of Young Accreting Stars

被引：0

作者：

Bouvier, Jerome ^{[1
]}

机构：

[1] Univ Grenoble Alpes, CNRS, IPAG, F-38000 Grenoble, France

来源：

NON-STABLE UNIVERSE: ENERGETIC RESOURCES, ACTIVITY PHENOMENA, AND EVOLUTIONARY PROCESSES | 2017年 / 511卷

关键词：

T-TAURI STARS; MAGNETOSPHERIC ACCRETION; MAGNETIZED STARS; MASS ACCRETION; AA-TAURI; FIELDS; LUP; I;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The evolution of disk hosting young stellar objects over the time frame 1-10 Myr is briefly reviewed. Emphasis is put on the evolution of mass accretion rate and stellar magnetic field properties, two central ingredients that dictate the nature of the star-disk interaction, i.e., how accretion proceeds from the inner disk edge to the central star, thus impacting its longer term evolution.

引用

页码：28 / 36

页数：9

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