The influence of new opacity data on the vertical structure of accretion disks

被引：0

作者：

Liu, BF

MeyerHofmeister, E

机构：

[1] MAX PLANCK INST ASTROPHYS, D-85740 GARCHING, GERMANY

[2] ACAD SINICA, YUNNAN OBSERV, KUNMING 650011, PEOPLES R CHINA

来源：

ASTRONOMY & ASTROPHYSICS | 1997年 / 328卷 / 01期

关键词：

accretion; accretion disk; instability; novae; cataclysmic variables;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Using the most recent opacity tables and the corresponding equation of state (EOS) data, we compute the vertical structure of accretion disks in cataclysmic variables, and give the new numerical results. We also present the resulting viscosity-surface density relation. We conclude that the improvement of opacity and EOS hardly influences the disk structure compared to the uncertainties connected with parameterization of viscosity and mixing length.

引用

页码：243 / 246

页数：4

共 16 条

[1] LOW-TEMPERATURE ROSSELAND OPACITIES [J].