Insights on the X-ray weak quasar phenomenon from XMM-Newton monitoring of PHL 1092-Reference-Cited by-同舟云学术

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Insights on the X-ray weak quasar phenomenon from XMM-Newton monitoring of PHL 1092

Published:2012-08-17 Issue:3 Volume:425 Page:1718-1737
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:Monthly Notices of the Royal Astronomical Society

Author:

Miniutti G.¹,Brandt W. N.,Schneider D. P.,Fabian A. C.²,Gallo L. C.³,Boller Th.⁴

Affiliation:

1. Centro de Astrobiología (CSIC-INTA); Dep. de Astrofísica; ESA; PO Box 78; E-28691; Villanueva de la Cañada; Madrid; Spain

2. Institute of Astronomy; Madingley Road; Cambridge; CB3 0HA

3. Department of Astronomy and Physics; Saint Mary's University; 923 Robie Street; Halifax; NS; B3H 3C3; Canada

4. Max-Planck-Institut für extraterrestrische Physik; Postfach 1312; 85741; Garching; Germany

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/425/3/1718/3012798/425-3-1718.pdf

Reference96 articles.

1. Inferences from a study of Fe II emission in radio-loud and radio-quiet quasars⋆

2. XMM-Newtondiscovery of a sharp spectral feature at ∼ 7 keV in the narrow-line Seyfert 1 galaxy 1H 0707−495

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3. XMM-Newton Observations of Two Archival X-Ray Weak Type 1 Quasars: Obscuration Induced X-Ray Weakness and Variability;The Astrophysical Journal;2023-09-01

4. Strong and Rapid X-Ray Variability of the Super-Eddington Accreting Quasar SDSS J081456.10+532533.5;The Astrophysical Journal;2023-06-01

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