2 CATACLYSMIC VARIABLES SIMILAR TO WZ-SAGITTAE

被引：48
作者：
BAILEY, J
机构：
[1] Hatfield Polytechnic Observatory, Bayfordbury House, Hertford,SGJ3 8LD, United Kingdom
来源：
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1979年 / 189卷 / 02期
关键词：
Astrophysics; -; Stars;
D O I：
10.1093/mnras/189.1.41P
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The cataclysmic variables UZ Boo and WX Cet both resemble WZ Sge in showing large outburst amplitudes (8 mag), slow declines from outbursts, and long intervals between outbursts. It is proposed that these three stars form a distinct sub-group of the dwarf novae and that they may all have similar binary structure. © Royal Astronomical Society • Provided by the NASA Astrophysics Data System.
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页码：P41 / P44
页数：4
相关论文
共 28 条
[1]  
Bailey J., 1975, Journal of the British Astronomical Association, V86, P30
[2]  
Bailey J., 1975, Journal of the British Astronomical Association, V85, P217
[3]  
BAILEY J, 1978, THESIS U SUSSEX
[4]   PERIODICITIES AND DISKS IN DWARF NOVAE [J].
BATH, GT .
NATURE-PHYSICAL SCIENCE, 1973, 246 (154) :84-87
[5]   ACCRETION MODEL OF DWARF NOVAE WITH APPLICATION TO Z CHAMAELEONTIS [J].
BATH, GT ;
EVANS, WD ;
PAPALOIZOU, J ;
PRINGLE, JE .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1974, 169 (03) :447-470
[6]  
BATH GT, 1976, STRUCTURE EVOLUTION, P173
[7]  
BOHUSZ E, 1979, INF B VAR STARS, P1583
[8]  
BORTLE JE, 1978, AAVSO96 CIRC
[9]  
BRUN A, 1957, PEREM ZVEZDY, V12, P18
[10]   DETERMINATION OF ORBITAL PARAMETERS OF WZ SAGITTAE [J].
FABIAN, AC ;
LIN, DNC ;
PAPALOIZOU, J ;
PRINGLE, JE .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1978, 184 (03) :835-841
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