Long-term monitoring of PKS 0558−504 with Swift: the disc-corona link

PKS 0558−504 is a highly-variable, X-ray-bright, radio-loud, narrow-line Seyfert 1 galaxy with super-Eddington accretion rate and extended jets that do not dominate the emission beyond the radio band. Therefore, this source represents an ideal laboratory to shed some light on the central engine in h...

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Bibliographic Details
Published in:Monthly notices of the Royal Astronomical Society 2013-08, Vol.433 (2), p.1709-1717
Main Authors: Gliozzi, M., Papadakis, I. E., Grupe, D., Brinkmann, W. P., Räth, C.
Format: Article
Language:English
Subjects:
Accretion disks
Atoms & subatomic particles
Corona
Stars & galaxies
Ultraviolet radiation
X-ray astronomy
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