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矮新星AB Dra中的吸积盘模型
引用本文:李宗云,丁月蓉.矮新星AB Dra中的吸积盘模型[J].天文学报,1995,36(4):385-393.
作者姓名:李宗云  丁月蓉
作者单位:南京大学天文系
摘    要:对矮新星AB Dra的最小二乘拟合表明,黑体吸积盘模型预言的连续谱能粗略地拟合该星在爆发期间的IUE观测,较小的偏差可以归因于光学薄气体的复合辐射或/和热斑的黑体辐射,拟合给出了一组吸积盘参量的合理值。

关 键 词:激变变星  吸积盘  紫外辐射  矮新星

ON THE ACCRETION DISK IN AB DRACONIS
Li Zong-yun, Zhu Ci-sheng, Ding Yue-rong.ON THE ACCRETION DISK IN AB DRACONIS[J].Acta Astronomica Sinica,1995,36(4):385-393.
Authors:Li Zong-yun  Zhu Ci-sheng  Ding Yue-rong
Abstract:In this paper the least-squares fit for dwarf nova AB Dra shows that the continuum predicted by the blackbody accretion disk model can roughly fit to the observed IVE data and the smaller deviation may be attributed to an appropriate amount of recombination radiation from optically thin gas or/and black body radiation from the hot spot.From the fitting we have obtained the reasonable values of some parameters of the disk and the system which it belongs to.
Keywords:Cataclysnic varibles  Accretion disk  Ultraviolet radiation  
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