Two-dimensional models of protoplanetary disk chemistry

被引：8
作者：
Millar, TJ [1 ]
Nomura, H [1 ]
Markwick, AJ [1 ]
机构：
[1] UMIST, Dept Phys, Manchester M60 1QD, Lancs, England
来源：
ASTROPHYSICS AND SPACE SCIENCE | 2003年 / 285卷 / 3-4期
关键词：
protoplanetary disks; astrochemistry;
D O I：
10.1023/A:1026129830938
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We have developed a two-dimensional model of a flared protoplanetary disk (PPD) incorporating a self-consistent treatment of gas and dust temperature, and a detailed treatment of the gas-phase chemistry as well as the freeze-out and desorption of material from dust grains. The results show that, in the inner 10 AU of the disk, the gas-phase abundances are dominated by material evaporated from dust grains. The surface layer of the disk shows many of the characteristics of photon-dominated regions.
引用
收藏
页码：761 / 768
页数：8
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