Structure in the ε Eridani dusty disk caused by mean motion resonances with a 0.3 Eccentricity planet at periastron

Astrophysical Journal

Volumn 578, Issue 2 II, 2002, Pages

  Quillen, A C ^a   Thorndike, Stephen ^a  

^a UNIVERSITY OF ROCHESTER   (United States)

Author keywords

Circumstellar matter; Planetary systems; Stars: individual ( Eridani)

Indexed keywords

EID: 0042262002     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/344708     Document Type: Article

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