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arXiv 1206.4845astro-ph.HE
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用双臂垂直p模振荡描述kHz QPO和HBO之间的频率相关性:无磁场的情况

An Attempt to Describe Frequency-Correlations among kHz QPOs and HBOs by Two-Armed Vertical p-mode Oscillations: Case of No Magnetic Field

Shoji kato

摘要:

本文研究了相对论圆盘中两臂($m=2$)垂直p模振荡的俘获。圆盘被假定为在垂直方向上是等温的,但是由于日冕的存在而在一定高度处被截断。同样的问题已经在以前的论文中研究过(Kato 2012 a)。然而,与前一篇文章不同,本文没有使用近似的振荡是几乎垂直的,而是限制在一个更简单的情况下,没有磁场。与前一篇论文一样,结果表明,两个基本振荡模式[在垂直方向上都是基频($n=1$),但在水平方向上一个是基频($n_{\rm r}=0$),另一个是第一泛音($n_{\rm r}=1$)]对应于双kHz QPO。第二,作为垂直方向上的第一泛音$(n=2)$和水平方向上的基波($n_{\rm r}=0$)的振荡模式将对应于Z源的水平分支振荡(HBO)。后者表明,Z源的水平分支是一个序列的温度变化的磁盘,其垂直厚度是强烈终止。温度从正常枝和水平枝之间的顶点开始依次升高。

英文摘要:

Trapping of two-armed ($m=2$) vertical p-mode oscillations in relativistic disks are examined. The disks are assumed to be isothermal in the vertical direction, but are truncated at a certain height by the presence of corona. The same issues have been examined in a previous paper (Kato 2012a). In this paper, unlike the previous paper, however, we do not use the approximation that the oscillations are nearly vertical, but limit to a simpler case of no magnetic field. As in the previous paper, the results suggest that the two basic oscillation modes [both are the fundamental ($n=1$) in the vertical direction but in the horizontal direction one is the fundamental ($n_{\rm r}=0$) and the other the first overtone ($n_{\rm r}=1$)] correspond to the twin kHz QPOs. Second, the oscillation mode which is the first overtone $(n=2)$ in the vertical direction and the fundamental in the horizontal direction ($n_{\rm r}=0$) will correspond to the horizontal branch oscillation (HBO) of Z-sources. The latter suggests that the horizontal branch of Z-sources is a sequence of temperature change in disks whose vertical thickness is strongly terminated. The temperature increases leftward along the sequence from the apex between normal and horizontal branches.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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