SWIFT J1753.5–0127: A Surprising Optical/X-Ray Cross-Correlation Function

SWIFT J1753.5–0127: A Surprising Optical/X-Ray Cross-Correlation Function
复制标题

DOI:
10.1086/590906
复制
发表时间:
2008-06
期刊:
The Astrophysical Journal Letters
影响因子:
--
通讯作者:
M. Durant;P. Gandhi;T. Shahbaz;A. Fabian;Jonathan M. Miller;V. Dhillon;T. Marsh
M. Durant;P. Gandhi;T. Shahbaz;A. Fabian;Jonathan M. Miller;V. Dhillon;T. Marsh
中科院分区:
其他
文献类型:
--
作者:
M. Durant;P. Gandhi;T. Shahbaz;A. Fabian;Jonathan M. Miller;V. Dhillon;T. Marsh

文献摘要

被引文献

相似文献

我们用RXTE和ULTRACAM对SWIFT J1753.5-0127进行了同步光学和X射线观测,而该系统一直处于相对明亮的低/硬状态。在互相关函数中,我们发现光发射有一个宽的负峰,领先X射线发射几秒,在正滞后处有一个较小的正峰。这与类似的有趣系统XTE J1118+480所看到的明显不同,这是第一次如此清晰地测量到这种相关函数。我们提出了一个物理场景的起源。
We have conducted simultaneous optical and X-ray observations of SWIFT J1753.5–0127 with RXTE and ULTRACAM, while the system persisted in its relatively bright low/hard state. In the cross-correlation function, we find that the optical emission, with a broad negative peak, leads the X-ray emission by a few seconds and has a smaller positive peak at positive lags. This is markedly different from what was seen for the similarly interesting system XTE J1118+480, and it is the first time that such a correlation function has been so clearly measured. We suggest a physical scenario for its origin.