The Role of Opacities in Calculating the Structure and Evolution of Protoplanetary Disks

被引：0

作者：

Calvet, Nuria ^{[1
]}

机构：

[1] Univ Michigan, Dept Astron, Ann Arbor, MI 48109 USA

来源：

WORKSHOP ON ASTROPHYSICAL OPACITIES | 2018年 / 515卷

关键词：

T-TAURI STARS; MOLECULAR-HYDROGEN; ACCRETION DISKS; CIRCUMSTELLAR DISKS; YOUNG OBJECTS; EMISSION; RADIATION; DATABASE; DUST; ULTRAVIOLET;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The most important heating agent of protoplanetary disks is absorption of radiation arising in the very active stellar atmosphere and in the accretion flows onto the star. Here, I give a brief review of the opacity mechanisms important in disks and of their current treatment.

引用

页码：231 / 240

页数：10

共 43 条

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