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XMM-Newton and Swift observations of the Seyfert 1 AGN NGC 5940
DOI: 10.1007/s10509-022-04082-1
Bibcode: 2022Ap&SS.367...51A
Adegoke, Oluwashina K.
Probing the physics of the accretion flow around active galactic nuclei (AGN) is crucial to understanding their emission mechanisms as well as being able to constrain the geometrical and variability properties of the different regions around them. The soft X-ray excess – usually observed below
2022
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Astrophysics and Space Science
XMM-Newton
0