Could the 55 Cancri planetary system really be in the 3:1 mean motion resonance?

Astrophysical Journal

Volumn 585, Issue 2 II, 2003, Pages

  Ji, Jianghui ^a,b   Kinoshita, Hiroshi ^c   Liu, Lin ^d   Li, Guangyu ^a,b  

^a CHINESE ACADEMY OF SCIENCES   (China)

^b CHINESE ACADEMY OF SCIENCES   (China)

^c NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^d NANJING UNIVERSITY   (China)

Author keywords

Celestial mechanics; Methods: n body simulations; Planetary systems; Stars: individual (55 Cancri, GJ 876, HD 12661, HD 82943, v Andromedae, 47 Ursae Majoris)

Indexed keywords

EID: 0038299825     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/374391     Document Type: Article

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