The Origin of The Soft X-Ray Excess in the Seyfert 1.5 Galaxy ESO 362-G18
Sign Up to like & getrecommendations! Published in 2021 at "Research in Astronomy and Astrophysics"
DOI: 10.1088/1674-4527/ac42c0
Abstract: We review the Seyfert 1.5 Galaxy ESO 362-G18 for exploring the origin of the soft X-ray excess. The Warm Corona and Relativistic Reflection models are two main scenarios to interpret the soft X-ray excess in… read more here.
Keywords: ray excess; corona; soft ray; warm corona ... See more keywords
Examining the physical conditions of a warm corona in active galactic nuclei accretion discs
Sign Up to like & getrecommendations! Published in 2019 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stz3294
Abstract: A warm corona at the surface of an accretion disc has been proposed as a potential location for producing the soft excess commonly observed in the X-ray spectra of active galactic nuclei (AGNs). In order… read more here.
Keywords: galactic nuclei; physical conditions; active galactic; accretion ... See more keywords