Flickering in FU Orionis

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© 2000. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Scott J. Kenyon et al 2000 ApJ 531 1028 DOI 10.1086/308515

0004-637X/531/2/1028

Abstract

We analyze new and published optical photometric data of FU Orionis, an eruptive pre-main-sequence star. The outburst consists of a 5.5 mag rise at B with an e-folding timescale of ∼50 days. The rates of decline at B and V are identical, 0.015 ± 0.001 mag yr-1. Random fluctuations superimposed on this decline have an amplitude of 0.035 ± 0.005 mag at V and occur on timescales of 1 day or less. Correlations between V and the color indices U-B, B-V, and V-R indicate that the variable source has the optical colors of a G0 supergiant. We associate this behavior with small-amplitude flickering of the inner accretion disk.

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10.1086/308515