WZ-SAGITTAE - RECENT OBSERVATIONS LEADING TO A MODEL FOR SUPER-HUMP PHENOMENA

被引：23

作者：

GILLILAND, RL ^{[1
]}

KEMPER, E ^{[1
]}

机构：

[1] UNIV CALIF SANTA CRUZ,LICK OBSERV,BOARD STUDIES ASTRON & ASTROPHYS,SANTA CRUZ,CA 95064

来源：

关键词：

D O I：

10.1086/157810

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：854 / 861

页数：8

共 25 条

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[7] HERBIG GH, 1978, COMMUNICATION
[8] Krzeminski W., 1971, Acta Astronomica, V21, P133
[9] BINARY STARS AMONG CATACLYSMIC VARIABLES .5. PHOTOELECTRIC + SPECTROSCOPIC OBSERVATIONS OF ULTRA-SHORT-PERIOD BINARY NOVA WZ SAGITTAE
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[J]. ASTROPHYSICAL JOURNAL, 1964, 140 (03) : 921 - &
[10] LIN DNC, 1979, COMMUNICATION