MAGNETIC OVERSTABILITY AS AN EXCITATION MECHANISM OF THE RAPID OSCILLATIONS OF AP STARS

被引：54

作者：

SHIBAHASHI, H

机构：

[1] UNIV COLORADO,NBS,JOINT INST LAB ASTROPHYS,BOULDER,CO 80302

[2] NBS,WASHINGTON,DC

来源：

关键词：

D O I：

10.1086/184160

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：L5 / L9

页数：5

共 9 条

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BORRA, EF ;

LANDSTREET, JD ;

MESTEL, L .

[2]

CHANDRASEKHAR S, 1961, HYDRODYNAMIC HYDROMA, P146

[3]

COX JP, 1984, UNPUB AP J

[4] THE STRUCTURE OF SUNSPOT PENUMBRAS .2. THEORETICAL [J].

DANIELSON, RE .

[5] THERMAL-CONVECTIVE INSTABILITY [J].

DEFOUW, RJ .

[6]

Dolez N., 1982, PULSATIONS CLASSICAL, P248

[7]

KATO S, 1966, PUBL ASTRON SOC JPN, V18, P374

[8] RAPIDLY OSCILLATING AP STARS [J].

KURTZ, DW .

[9]

KURTZ DW, 1983, PREPRINT