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【9.27】2017年高能所粒子天体中心系列学术报告 # 5:Supersoft AGNs: signature of super Eddington accretion, IMBH, TDE or new AGN spectral state?
2017-09-27 | 【

  时间:今天上午10:00

  地点:报告厅406

  报告人:舒新文(安徽师范大学物理系)

  主持人:谭颖

  题目:Supersoft AGNs: signature of super Eddington accretion, IMBH, TDE or new AGN spectral state?

  摘要:Supersoft AGNs are a new class of AGNs which lack significant hard X-ray emission above ~2 keV. They may host intermediate mass black holes (IMBH) accreting in a poorly explored regime of parameter space, such as super Eddingtong accretion and extreme coronal condition. Their X-ray spectra are dominated by a soft thermal component, a form similar to disk blackbody emission in stellar-mass BHs in their high/soft state. Though only three supersoft AGNs are reported to date, they show distinct X-ray variability behavior, some of them could be associated with TDE.

  In this talk, I will present the multi-wavelength characteristics of RX J1301.9+2746, the most distinct source of this kind. In particular, I will show our follow-up JVLA observations which reveal fast intraday radio variability, confining its origin likely from a compact jet. Such the unexpected presence of jets in a supersoft AGN challenges canonical theories of jet formation. All the results suggest that this AGN is an ideal laboratory for studying the universality of accretion/ejection coupling in BH accreting systems.

  个人简介:

  2010年博士毕业于中国科技大学,2010.6-2013.6,中国科技大学博士后、副研究员。

  2013.6-2015.3 法国原子能中心(CEA)博士后,2015.3-至今 安徽师范大学教授。主要从事

  AGN和高红移星系的研究,已发表论文50余篇(第一/通讯作者12篇,大多为ApJ),

  被同行引用1200余次。


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