Origin of chromatic features in multiple quasars
Atsunori YoneharaAstronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg, Mönchhofstraße 12-14, Heidelberg 69120, GermanyHiroyuki HirashitaCenter for Computational Science, University of Tsukuba, Tennodai 1-1-1, Tsukuba, Ibaraki 305-8577, Japan e-mail: [email protected]P. RichterArgelander-Institut für Astronomie, Universität Bonn, Auf dem Hügel 71, 53121 Bonn, Germany
2007en
ABI
Annotatsiya
Aims.In some of lensed quasars, color differences between multiple images are observed at optical/near-infrared wavelengths. There are three possible origins for the color differences: intrinsic variabilities of quasars, differential dust extinction, and quasar microlensing. We examine how these possible scenarios can reproduce the observed chromaticity.
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