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首页> 外文期刊>Astrophysics and space science >Transient X-ray sources in the field of the unidentified gamma-ray source TeV J2032+4130 in Cygnus
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Transient X-ray sources in the field of the unidentified gamma-ray source TeV J2032+4130 in Cygnus

机译:天鹅座中身份不明的伽马射线源TeV J2032 + 4130的瞬态X射线源

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We present an analysis of Chandra ACIS observations of the field of TeV J2032+4130, the first unidentified TeV source, detected serendipitously by HEGRA. This deep (48.7 ks) observation of the field follows up on an earlier 5 ks Chandra director's discretionary observation. Of the numerous point-like X-ray sources in the field, the brightest are shown to be a mixture of early and late-type stars. We find that several of the X-ray sources are transients, exhibiting rapid increases in count rates by factors 3-10, and similar in nature to the one, hard absorbed transient source located in the earlier Chandra observation of the field. None of these transient sources are likely to correspond to the TeV source. Instead, we identify a region of diffuse X-ray emission within the error circle of the TeV source and consider its plausible association.
机译:我们介绍了Chandra ACIS对TeV J2032 + 4130(第一个未识别的TeV来源)领域的观测结果的分析,这是由HEGRA偶然发现的。对该场的深入观测(48.7 ks)跟随了钱德拉(Chandra)导演先前5 ks的酌情观测结果。在该领域的众多点状X射线源中,最亮的是早期和晚期恒星的混合物。我们发现,一些X射线源是瞬态的,其计数率迅速增加3-10倍,并且本质上与位于该领域早期钱德拉观测中的一个硬吸收的瞬态源相似。这些瞬态源都不可能与TeV源相对应。取而代之的是,我们在TeV源的误差圈内确定了X射线扩散区域,并考虑了其合理的关联。

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