Evolution and Dispersal of Protoplanetary Disks

被引：0
|
作者：
Sicilia-Aguilar, A. [1 ]
Henning, Th. [1 ]
Juhasz, A. [1 ]
Bouwman, J. [1 ]
Hartmann, L. [2 ]
Watson, D. [3 ]
机构：
[1] Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany
[2] Univ Michigan, Ann Arbor, MI 48109 USA
[3] Univ Rochester, Dept Phys & Astron, Rochester, NY 14627 USA
来源：
COOL STARS, STELLAR SYSTEMS AND THE SUN | 2009年 / 1094卷
关键词：
Stars: Formation; Planetary systems: Protoplanetary disks; Accretion disks; INTERSTELLAR SILICATE MINERALOGY; ACCRETION; DUST; PLANET; PHOTOEVAPORATION; GROWTH; GRAINS; DISCS; STEPS; GAS;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Multiwavelength studies of evolved protoplanetary disks around solar-type and low-mass stars reveal a general trend of changes in the IR excesses, accretion rates, and silicate features, suggesting grain growth/settling, photoevaporation, and maybe the formation of planetesimals and planets. Nevertheless within the average-behavior picture of disk evolution, we observe strong variations between individuals, that may be related to different initial conditions, different environments, and the presence of companions.
引用
收藏
页码：23 / +
页数：2
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