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WZ Sagittae - an old dwarf nova
Meyer-Hofmeister, E1; Meyer, F1; Liu BF(刘碧芳)2
发表期刊ASTRONOMY & ASTROPHYSICS
1998-11
卷号339期号:2页码:507-517
产权排序第2完成单位
收录类别SCI
关键词Accretion Disks Cataclysmic Variables Stars : Individual : Wz Sge X-rays : Stars Stars : Coronae
摘要We model the evolution of the accretion disk of WZ Sagittae during the long quiescence. We find that the large amount of mass in the disk derived from the outburst luminosity is a severe constraint and demands values of alpha(c) approximate to 0.001 in contradiction to some recent suggestions. We include in our computations the formation of an inner disk hole and the growth of the disk due to redistribution of angular momentum. We find a new mode of disk evolution. The disk is quasi-stationary. Only about half of the mass transfered from the companion star flows through the disk, the other half is needed to build up the steadily growing outer disk. When the 3:1 resonance radius is reached the disk growth ends. From then on all transferred matter flows inward, the surface density increases, leading to an outburst within a few years. We predict superhumps at low luminosity during this last phase. We discuss X-rays expected, the white dwarf mass and distance to WZ Sagittae.
语种英语
学科领域Astronomy & Astrophysics
文章类型Article
ISSN0004-6361
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WOS记录号WOS:000077014200025
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]DISK BOUNDARY-LAYERS ; X-RAY-EMISSION ; CATACLYSMIC VARIABLES ; ACCRETION DISK ; WHITE-DWARF ; OUTBURSTS ; MODEL ; SGE ; EVAPORATION ; SUPERHUMPS
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被引频次:38[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/4925
专题高能天体物理研究组
通讯作者Meyer-Hofmeister, E
作者单位1.Max-Planck-Institut fur Astrophysik, Karl-Schwarzschildstrasse 1, D-85740 Garching, Germany
2.Yunnan Observatory, Academia Sinica. P.O.Box 110, Kunming 650011, P.R. China
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Meyer-Hofmeister, E,Meyer, F,Liu BF. WZ Sagittae - an old dwarf nova[J]. ASTRONOMY & ASTROPHYSICS,1998,339(2):507-517.
APA Meyer-Hofmeister, E,Meyer, F,&Liu BF.(1998).WZ Sagittae - an old dwarf nova.ASTRONOMY & ASTROPHYSICS,339(2),507-517.
MLA Meyer-Hofmeister, E,et al."WZ Sagittae - an old dwarf nova".ASTRONOMY & ASTROPHYSICS 339.2(1998):507-517.
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