DARK MATTER AND THE SUPPRESSION OF STELLAR CORE CONVECTION

被引：26

作者：

BOUQUET, A

SALATI, P

机构：

[1] UNIV CALIF BERKELEY LAWRENCE BERKELEY LAB,CTR PARTICLE ASTROPHYS,BERKELEY,CA 94720

[2] UNIV CALIF BERKELEY,DEPT ASTRON & PHYS,BERKELEY,CA 94720

来源：

关键词：

D O I：

10.1086/168009

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：284 / 288

页数：5

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[2]

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[4]

BOUQUET A, 1987, IN PRESS ASTR AP

[5]

CASSE M, 1987, COMMUNICATION

[6]

CLAYTON DD, 1968, PRINCIPLES STELLAR E, P230

[7]

CLAYTON DD, 1968, PRINCIPLES STELLAR E, P362

[8]

DELUCA EE, 1989, IN PRESS AP J

[9] MAIN-SEQUENCE EVOLUTION WITH EFFICIENT CENTRAL ENERGY-TRANSPORT [J].

FAULKNER, J ;

SWENSON, FJ .

[10] WEAKLY INTERACTING, MASSIVE PARTICLES AND THE SOLAR NEUTRINO FLUX [J].

FAULKNER, J ;

GILLILAND, RL .