Observations of a transient X-ray source with a period of 104 s

Observations of a transient X-ray source with a period of 104 s
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DOI：
10.1038/256628a0
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发表时间：
1975-08
期刊：
Nature
影响因子：
64.8
通讯作者：
F. Rosenberg;C. Eyles;G. Skinner;A. Willmore
F. Rosenberg;C. Eyles;G. Skinner;A. Willmore
中科院分区：
综合性期刊1区
文献类型：
--
作者：
F. Rosenberg;C. Eyles;G. Skinner;A. Willmore

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在Ariel V对蟹状星云的常规观测中，实验A，旋转调制准直器（RMC），发现了一个新的x射线源A0535+26。在4月13日的第一次观测中，光源才被探测到，在16天的观测中，它的亮度几乎是蟹状星云强度的两倍（在3-7 keV范围内）。光源周期性变化，周期为104 s，在3-7 keV范围内具有非常平坦的频谱。
DURING routine observations of the Crab Nebula by Ariel V, experiment A, the rotation modulation collimator (RMC), discovered a new X-ray source A0535+26. The source was just detectable during the first observation on April 13, and during the 16 d of observation was seen to brighten to nearly twice the Crab's intensity (in the 3–7 keV range). The source varies periodically, with a period of 104 s, and has a very flat spectrum in the 3–7 keV range.