G-MODE INSTABILITY IN THE MAIN-SEQUENCE B-TYPE STARS

被引:0
作者
DZIEMBOWSKI, WA [1 ]
MOSKALIK, P [1 ]
PAMYATNYKH, AA [1 ]
机构
[1] PK SHTERNBERG ASTRON INST,MOSCOW 109017,RUSSIA
来源
PULSATION, ROTATION AND MASS LOSS IN EARLY-TYPE STARS | 1994年 / 162期
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中图分类号
P1 [天文学];
学科分类号
0704 ;
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页码:69 / 69
页数:1
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