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A Correlated Optical-Infrared Outburst of Mrk 744: Strong Evidence for Thermal Dust Reverberation

Published online by Cambridge University Press:  12 April 2016

B. Nelson*
Affiliation:
Departments of Physics and Astronomy, UCLA, Los Angeles, CA 90095-1562, USA

Abstract

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Simultaneous optical and infrared monitoring of a sample of 50 Seyfert 1 galaxies and quasars has revealed an outburst of the active galaxy Markarian 744. Cross-correlation analysis indicates that the IR lags the optical light curve by roughly one month. A simple model developed by the author can fully explain the IR variability of this object in terms of thermal dust reverberation.

Type
VI. The Narrow-Line Regions and Beyond
Copyright
Copyright © Astronomical Society of the Pacific 1997

References

Clavel, J., Wamsteker, W., & Glass, I.S. 1989, ApJ, 337, 236.Google Scholar
Gezari, D.Y., Schmitz, M., Pitts, P.S. & Mead, J.M. 1993, Catalog of Infrared Observations, Third Edition, NASA Reference Publication 1294.Google Scholar
McLean, I. 1994, in Infrared Astronomy With Arrays: The Next Generation, ed. McLean, I.S. (Boston: Kluwer), 391.Google Scholar
Nelson, B., & McLean, I.S. 1996, PASP, in preparation.Google Scholar
Nelson, B.O. 1996, ApJ, 465, L87.CrossRefGoogle Scholar