Fig. 3 from Differential Rotation of ϵ Eridani Detected by MOST

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Differential Rotation of ϵ Eridani Detected by MOST

Authors: Bryce Croll, Gordon A. H. Walker, Rainer Kuschnig, Jaymie M. Matthews, Jason F. Rowe, Andrew Walker, Slavek M. Rucinski, Artie P. Hatzes, William D. Cochran, Russell M. Robb, David B. Guenther, Anthony F. J. Moffat, Dimitar Sasselov, and Werner W. Weiss

Croll et al. 2006 The Astrophysical Journal 648 607.

Provider: AAS Journals

Caption: Fig. 3.

Amplitude spectra of the model (dotted line) of Fig. 2 and of the residuals from the model (solid line), demonstrating that no signal remains in the residuals over the range of rotational rates (﹩0.088\pm 0.012﹩ cycles day−1) expected for Eri.

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