Confirmation of the nature of the absorber in IRAS 09104+4109
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/430/4/2943/3860312/stt097.pdf
Reference22 articles.
1. The 6.4-keV fluorescent iron line from cluster cooling flows
2. Compton-Thick AGN: The Dark Side of the X-Ray Background
3. Optical integral field spectroscopy and ROSAT X-ray imaging of IRAS 09104 + 4109
4. ROSAT HRI observations of IRAS P09104+4109: a massive cooling flow
5. Fe K emission from the hidden quasar IRAS P09104+4109
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1. NuSTAR reveals that the heavily obscured nucleus of NGC 2785 was the contaminant of IRAS 09104+4109 in the BeppoSAX/PDS hard X-rays;Astronomy & Astrophysics;2018-10-30
2. THE GEOMETRY OF THE INFRARED AND X-RAY OBSCURER IN A DUSTY HYPERLUMINOUS QUASAR;The Astrophysical Journal;2016-10-27
3. FORMATION OF RAMAN SCATTERING WINGS AROUND Hα, Hβ, AND PAαIN ACTIVE GALACTIC NUCLEI;The Astrophysical Journal;2015-11-20
4. Compton thick AGN in the XMM-COSMOS survey;Astronomy & Astrophysics;2015-01
5. Modelling the X-ray polarimetric signatures of complex geometry: the case study of the 'changing look' active galactic nucleus NGC 1365;Monthly Notices of the Royal Astronomical Society;2013-10-01
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