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准周期振荡(QPO)天体GX5-1的双分支谱的唯象分析
引用本文:尤峻汉,陆埮,冯珑珑,晏明.准周期振荡(QPO)天体GX5-1的双分支谱的唯象分析[J].中国天文和天体物理学报,1990(4).
作者姓名:尤峻汉  陆埮  冯珑珑  晏明
作者单位:中国科技大学天体物理中心,南京大学天文系,中国科技大学天体物理中心,中国科技大学天体物理中心 南京大学天文系
摘    要:本文对小质量X射线双星的准周期振荡的差频模型做了修正和补充。修正的要点是:要考虑柱吸积过程中的粘滞阻尼。由此即可成功地解释QPO天体GX5-1的双分支谱特性。

关 键 词:X射线双星  准周期振荡  双分支谱

A Phenomenological Analysis of the Spectral Bimodality in the QPO Object GX 5-1
You Junhan Lu TanFeng Longlong Yan MingCenter for Astrophysics,Univ. of Set. and Tec,of China,HeifeiAstronomy.A Phenomenological Analysis of the Spectral Bimodality in the QPO Object GX 5-1[J].Chinese Journal of Astronomy and Astrophysics,1990(4).
Authors:You Junhan Lu TanFeng Longlong Yan MingCenter for Astrophysics  Univ of Set and Tec  of China  HeifeiAstronomy
Abstract:Some corrections and improvements to the beat frequency model for the quasi-periodic oscillation phenomenon in X-rays binaries have been made in this paper. The main point is that the viscous damping in the column accretion process has been taken into consideration, which successfully accounts for the two-branch spectrum behaviour unexplained by the previous beat frequency model.
Keywords:A-ray binaries-QPO phenomenon-Speciral bimodality
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