3D HYDRODYNAMICS AND RADIATIVE TRANSFER

被引：0
|
作者：
Boss, A. P. [1 ]
机构：
[1] Carnegie Inst Washington, DTM, Washington, DC 20015 USA
来源：
CELESTIAL MECHANICS & DYNAMICAL ASTRONOMY | 1988年 / 45卷 / 1-3期
关键词：
D O I：
10.1007/BF01228984
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Finite difference codes for the solution of the fully three dimensional equations of hydrodynamics, self-gravitation, and radiative transfer have been developed for use on relatively modest computers. Originally developed to study the collapse and fragmentation of protostellar clouds, this family of codes has been used to study a variety of astrophysical problems, with a particular emphasis on cosmogonical issues.
引用
收藏
页码：85 / 88
页数：4
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