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dc.creatorPoindexter, Shawn
dc.creatorKochanek, Christopher S.
dc.date.accessioned2011-03-15T19:30:50Z
dc.date.available2011-03-15T19:30:50Z
dc.date.issued2010-03-20
dc.identifier.citationShawn Poindexter and Christopher S. Kochanek, "Microlensing Evidence That a Type 1 Quasar is Viewed Face-On," The Astrophysical Journal 712, no. 1 (2010), doi:10.1088/0004-637X/712/1/668en_US
dc.identifier.issn1538-4357
dc.identifier.urihttp://hdl.handle.net/1811/48295
dc.description.abstractUsing a microlensing analysis of 11 years of OGLE V-band photometry of the four image gravitational lens Q2237+0305, we measure the inclination i of the accretion disk to be cos i > 0.66 at 68% confidence. Very edge on (cos i < 0.39) solutions are ruled out at 95% confidence. We measure the V-band radius of the accretion disk, defined by the radius where the temperature matches the monitoring band photon emission, to be R_V = 5.8^+3.8_–2.3 × 10^15 cm assuming a simple thin disk model and including the uncertainties in its inclination. The projected radiating area of the disk remains too large to be consistent with the observed flux for a T α R^–3/4 thin disk temperature profile. There is no strong correlation between the direction of motion (peculiar velocity) of the lens galaxy and the orientation of the disk.en_US
dc.language.isoen_USen_US
dc.publisherAmerican Astronomical Societyen_US
dc.subjectgravitational lensing: microen_US
dc.subjectmethods: numericalen_US
dc.subjectquasars: individual (Q2237+0305)en_US
dc.titleMicrolensing Evidence That a Type 1 Quasar is Viewed Face-Onen_US
dc.typeArticleen_US
dc.identifier.doi10.1088/0004-637X/712/1/668
dc.identifier.osuauthorkochanek.1
dc.identifier.osuauthorpoindexter.22


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