The Structure and Evolution of Protoplanetary Disks: an Infrared and Submillimeter View

被引：0
|
作者：
Cieza, Lucas A. [1 ]
机构：
[1] Univ Diego Portales, Nucleo Astron, Santiago, Chile
来源：
YOUNG STARS & PLANETS NEAR THE SUN | 2016年 / 10卷 / 314期
关键词：
protoplanetary disks; infrared: planetary systems; submillimeter: planetary systems; CIRCUMSTELLAR DUST DISKS; GIANT PLANET FORMATION; SPITZER C2D SURVEY; TRANSITION; GAS; ACCRETION;
D O I：
10.1017/S1743921315006249
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Circumstellar disks are the sites of planet formation, and the very high incidence of extrasolar planets implies that most of them actually form planetary systems. Studying the structure and evolution of protoplanetary disks can thus place important constraints on the conditions, timescales, and mechanisms associated with the planet formation process. In this review, we discuss observational results from infrared and submillimeter wavelength studies. We review disk lifetimes, transition objects, disk demographics, and highlight a few remarkable results from ALMA Early Science observations. We finish with a brief discussion of ALMA's potential to transform the field in near future.
引用
收藏
页码：128 / 134
页数：7
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