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2002ApJ...578L.149Q - Astrophys. J., 578, L149-L152 (2002/October-3)
Structure in the ε eridani dusty disk caused by mean motion resonances with a 0.3 eccentricity planet at periastron.
QUILLEN A.C. and THORNDIKE S.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): Stars: Circumstellar Matter - Stars: Planetary Systems - Stars: Individual: Constellation Name: ε Eridani
Simbad objects: 6
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