X-Ray Microlensing of Bright Quasars
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/pasj/article-pdf/53/3/387/4405986/pasj53-0387.pdf
Reference41 articles.
1. Thermal equilibria of accretion disks
2. Imaging a Quasar Accretion Disk with Microlensing
3. Blandford R. D. Hogg D. W. 1995, in IAU Symp. 173, Astrophysical Application of Gravitational Lensing, ed. Kochanek C.S. Hewitt J. N. (Dordrecht: Kluwer), 355
4. Laboratory detection of X-ray fringes with a grazing-incidence interferometer
5. Flux variations of QSO 0957 + 561 A, B and image splitting by stars near the light path
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1. Amplification and variability of the AGN X-ray emission due to microlensing;Astronomische Nachrichten;2006-12
2. A Study of the Correlation between the Amplification of the Fe Kα Line and the X‐Ray Continuum of Quasars due to Microlensing;The Astrophysical Journal;2006-02
3. Size Is Everything: Universal Features of Quasar Microlensing with Extended Sources;The Astrophysical Journal;2005-08
4. Contribution of Microlensing to X-ray Variability of Distant QSOs;Proceedings of the International Astronomical Union;2004-07
5. On the contribution of microlensing to X-ray variability of high-redshifted QSOs;Astronomy & Astrophysics;2004-06
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