Published in
American Astronomical Society, Astrophysical Journal, 2(578), p. L149-L152, 2002
DOI: 10.1086/344708
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Structure in the ε Eridani Dusty Disk Caused by Mean Motion Resonances with a 0.3 Eccentricity Planet at Periastron
Journal article published in 2002 by
A. C. Quillen 
,
Stephen Thorndike
,
Stephen Thorndike
This paper was not found in any repository, but could be made available legally by the author.
Full text: Unavailable
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