ENERGY-TRANSFER IN CONTACT BINARY-SYSTEMS

被引:27
作者
ALISTAIRROBERTSON, J
机构
[1] Astronomy Centre, Physics Building, University of Sussex, Falmer, Brighton,BN1 9QH, United Kingdom
关键词
Astrophysics; -; NASA; Systems; (metallurgical);
D O I
10.1093/mnras/192.2.263
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A simple model for the transfer of energy by steady circulation within the envelope of a contact binary system is presented. The model describes the fully compressible, two-dimensional flow of a perfect gas within a rectangular region in a uniform gravitational field. The region is heated non-uniformly from below. Coriolis forces are neglected but the interaction of the circulation with convection is discussed briefly. Numerical solutions of the linearized equations of the problem are discussed in detail, and the results of some non-linear calculations are also presented. The influence of alternative boundary conditions is examined. © 1980 Royal Astronomical Society. Provided by the NASA Astrophysics Data System.
引用
收藏
页码:263 / 281
页数:19
相关论文
共 27 条
[1]  
Du Fort E.C., 1953, MATH TABLES OTHER AI, V7, P135, DOI [DOI 10.2307/2002754, 10.1090/S0025-5718-1953-0059077-7]
[2]   CONVECTIVE INSTABILITY IN A COMPRESSIBLE ATMOSPHERE .2. [J].
GOUGH, DO ;
MOORE, DR ;
SPIEGEL, EA ;
WEISS, NO .
ASTROPHYSICAL JOURNAL, 1976, 206 (02) :536-542
[3]  
Graham E., 1977, Proceedings of the Colloquium No.38 of the International Astronomical Union, P151
[4]   ONSET OF COMPRESSIBLE CONVECTION [J].
GRAHAM, E ;
MOORE, DR .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1978, 183 (03) :617-632
[5]   NUMERICAL-SIMULATION OF 2-DIMENSIONAL COMPRESSIBLE CONVECTION [J].
GRAHAM, E .
JOURNAL OF FLUID MECHANICS, 1975, 70 (AUG26) :689-703
[6]  
HAZLEHURST J, 1973, ASTRON ASTROPHYS, V24, P379
[7]  
HAZLEHURST J, 1978, ASTRON ASTROPHYS, V62, pL9
[8]  
KIPPENHAHN R, 1979, ASTRON ASTROPHYS, V75, P281
[9]   STRUCTURE OF CONTACT BINARIES [J].
LUCY, LB .
ASTROPHYSICAL JOURNAL, 1968, 151 (3P1) :1123-&
[10]   ENERGY-TRANSFER IN CONTACT BINARIES [J].
MOSES, AP .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1976, 176 (01) :161-174