Fig. 2 from Differential Rotation of ϵ Eridani Detected by MOST

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

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. 2.

Top: epsilon Eri spots (Table 3) as seen from the line of sight (left) and the visible pole (right). Middle: The light curve of Fig. 1, with a linear trend removed. The solid line is the model from Table 3. The dashed line indicates the unspotted intensity of the star (﹩U=1.0000﹩). Bottom: Residuals from the model on the same scale.

Other Images in This Article

Copyright and Terms & Conditions