首页> 外文期刊>The Astrophysical journal >DISCOVERY OF HARD X-RAY DELAYS IN THE X-RAY EMISSION OF THE SEYFERT 1 GALAXY MARKARIAN 110: POSSIBLE EVIDENCE OF COMPTONIZATION
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DISCOVERY OF HARD X-RAY DELAYS IN THE X-RAY EMISSION OF THE SEYFERT 1 GALAXY MARKARIAN 110: POSSIBLE EVIDENCE OF COMPTONIZATION

机译:SEYFERT 1 GALAXY MARKARIAN 110的X射线发射中的硬X射线延迟的发现:可能的证词化

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摘要

We report the discovery of hard X-ray delays in the X-ray emission of the Seyfert 1 galaxy Mrk 110, based on a long XMM-Newton observation. Cross-correlation between the X-ray light curves of different energy bands reveals an energy-dependent delay ranging from a few minutes to an hour. We find that the energy spectrum can be modeled by Comptonization of disk blackbody photons. The energy-dependent delay can be modeled as due to the effect of Comptonization in a hot plasma confined within 10 Schwarzschild radii of the black hole. We discuss our results in the context of inverse Comptonization of the soft photons by highly energetic plasma.
机译:我们报告了基于长期XMM-牛顿观测的塞弗特1号星系Mrk 110的X射线发射中的硬X射线延迟发现。不同能带的X射线光曲线之间的互相关揭示了取决于能量的延迟,范围从几分钟到一个小时。我们发现能谱可以通过盘黑体光子的Comptonization建模。取决于能量的延迟可以建模为归因于在黑洞的10 Schwarzschild半径内限制的热等离子体中的Comptonization效应。我们在通过高能等离子体使软光子逆Comptonization的背景下讨论我们的结果。

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