Semiconvection and overshooting: Schwarzschild and Ledoux criteria revisited

被引:10
作者
Canuto, VM
机构
[1] NASA, Goddard Inst Space Studies, New York, NY 10025 USA
[2] Columbia Univ, Dept Appl Phys, New York, NY 10027 USA
关键词
convection; stars : interiors; turbulence;
D O I
10.1086/312654
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We show that the Schwarzschild formalism, if accepted as the description of the structure of a semiconvective region, necessarily implies overshooting. The Ledoux formalism (if accepted) can be used without overshooting, provided a new relation for the mixing-length parameter or is satisfied. Should the latter not be satisfied, the Ledoux formalism would also require overshooting, that is, a nonlocal convection model.
引用
收藏
页码:L113 / L115
页数:3
相关论文
共 10 条
[1]   Turbulence in stars. III. Unified treatment of diffusion, convection, semiconvection, salt fingers, and differential rotation [J].
Canuto, VM .
ASTROPHYSICAL JOURNAL, 1999, 524 (01) :311-340
[2]   Double-diffusive mixing-length theory, semiconvection and massive star evolution [J].
Grossman, SA ;
Taam, RE .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1996, 283 (04) :1165-1178
[3]  
LANGER N, 1985, ASTRON ASTROPHYS, V145, P179
[4]  
LEDOUX P, 1947, ASTROPHYS J, V105, P305
[5]   HYDRODYNAMICS OF SEMICONVECTION [J].
MERRYFIELD, WJ .
ASTROPHYSICAL JOURNAL, 1995, 444 (01) :318-337
[6]   INTERNAL STRUCTURE AND EVOLUTION OF VERY MASSIVE STARS [J].
SAKASHITA, S ;
HAYASHI, C .
PROGRESS OF THEORETICAL PHYSICS, 1959, 22 (06) :830-834
[7]   EVOLUTION OF VERY MASSIVE STARS [J].
SCHWARZSCHILD, M ;
HARM, R .
ASTROPHYSICAL JOURNAL, 1958, 128 (02) :348-360
[8]   STELLAR EVOLUTION IN BLUE POPULOUS CLUSTERS OF THE SMALL MAGELLANIC CLOUD AND THE PROBLEMS OF ENVELOPE SEMICONVECTION AND CONVECTIVE CORE OVERSHOOTING [J].
STOTHERS, RB ;
CHIN, CW .
ASTROPHYSICAL JOURNAL, 1992, 390 (01) :136-143
[9]   GALACTIC STARS APPLIED TO TESTS OF THE CRITERION FOR CONVECTION AND SEMICONVECTION IN AN INHOMOGENEOUS STAR [J].
STOTHERS, RB ;
CHIN, CW .
ASTROPHYSICAL JOURNAL, 1994, 431 (02) :797-805
[10]   Hydrogen flux in the semiconvection zone of the massive main sequence stars [J].
Umezu, M .
ASTROPHYSICS AND SPACE SCIENCE, 1998, 259 (04) :343-354