Constraining black hole masses in low-accreting active galactic nuclei using X-ray spectra
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/443/1/72/4282968/stu1024.pdf
Reference90 articles.
1. Supermassive black hole mass measurements for NGC 1300 and 2748 based on Hubble Space Telescope emission-line gas kinematics
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4. HSTSTIS Spectroscopy of the Triple Nucleus of M31: Two Nested Disks in Keplerian Rotation around a Supermassive Black Hole
5. HOW COMPLEX IS THE OBSCURATION IN ACTIVE GALACTIC NUCLEI? NEW CLUES FROM THESUZAKUMONITORING OF THE X-RAY ABSORBERS IN NGC 7582
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1. Comparing indirect methods for black hole masses in AGN: The good, the bad, and the ugly;Monthly Notices of the Royal Astronomical Society;2023-12-23
2. Coronal properties of low-accreting AGNs using Swift, XMM–Newton, and NuSTAR observations;Monthly Notices of the Royal Astronomical Society;2023-07-17
3. Assessing indirect methods to determine black hole masses using NGC 4151;Monthly Notices of the Royal Astronomical Society;2023-03-10
4. FRAMEx. III. Radio Emission in the Immediate Vicinity of Radio-quiet AGNs;The Astrophysical Journal;2022-08-31
5. Observational hints on the torus obscuring gas behaviour through X-rays with NuSTAR data;Monthly Notices of the Royal Astronomical Society;2021-12-27
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