BINARY STARS AMONG CATACLYSMIC VARIABLES .2. NOVA WZ SAGITTAE - A POSSIBLE RADIATOR OF GRAVITATIONAL WAVES

被引：149

作者：

KRAFT, RP

MATHEWS, J

GREENSTEIN, JL

机构：

来源：

ASTROPHYSICAL JOURNAL | 1962年 / 136卷 / 01期

关键词：

D O I：

10.1086/147381

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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页码：312 / &

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[2] THE BINARY SYSTEM NOVA DQ HERCULIS .1. THE SPECTRUM AND RADIAL VELOCITY DURING THE ECLIPSE CYCLE
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[3] GREENSTEIN JL, 1958, ENCYCL PHYS, V50, P161
[4] BINARY STARS AMONG CATACLYSMIC VARIABLES .1. U GEMINORUM STARS (DWARF NOVAE)
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[J]. ASTROPHYSICAL JOURNAL, 1962, 135 (02) : 408 - &
[5] KRAFT RP, 1961, SCIENCE, V134, P1433
[6] THE BINARY SYSTEM NOVA DQ HERCULIS .2. AN INTERPRETATION OF THE SPECTRUM DURING THE ECLIPSE CYCLE
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[J]. ASTROPHYSICAL JOURNAL, 1959, 130 (01) : 110 - 122
[7] NOVA WZ SAGITTAE - AN EXTREMELY SHORT-PERIOD ECLIPSING BINARY
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[J]. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 1962, 74 (436) : 66 - 69
[8] THE SPECTRA OF NOVAE NEAR MINIMUM
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[9] [No title captured]