The Nuclear X-Ray Emission-line Structure in NGC 2992 Revealed byChandra-HETGS
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/840/i=2/a=120/pdf
Reference43 articles.
1. Physical Conditions in the Seyfert Galaxy NGC 2992
2. The 1–200 keV X‐Ray Spectrum of NGC 2992 and NGC 3081
3. High-resolution X-ray spectroscopy and imaging of Mrk 573
4. The soft X-ray/NLR connection: a single photoionized medium?
5. The nature and origin of Seyfert warm absorbers
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1. Revisiting the Circumnuclear X-Ray Emission of NGC 2992 in a Historically Low State;The Astrophysical Journal;2022-10-01
2. Localizing narrow Fe Kαemission within bright AGN;Astronomy & Astrophysics;2022-08
3. FRAMEx. II. Simultaneous X-Ray and Radio Variability in Active Galactic Nuclei—The Case of NGC 2992;The Astrophysical Journal;2022-03-01
4. The Eddington ratio-dependent ‘changing look’ events in NGC 2992;Monthly Notices of the Royal Astronomical Society;2021-09-11
5. The Correlated Response of the Narrow FeKα Emission Line to the Primary Continuum Changes in the Seyfert Galaxy NGC 2992;Research Notes of the AAS;2021-02-01
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