55 Cancri: Stellar astrophysical parameters, a planet in the habitable zone, and implications for the radius of a transiting super-earth

Astrophysical Journal

Volumn 740, Issue 1, 2011, Pages

  Von Braun, Kaspar ^a   Tabetha, S Boyajian ^b   Ten Brummelaar, Theo A ^c   Kane, Stephen R ^a   Van Belle, Gerard T ^d   Ciardi, David R ^a   Raymond, Sean N ^e,f   López Morales, Mercedes ^g,h   McAlister, Harold A ^b   Schaefer, Gail ^c   Ridgway, Stephen T ⁱ   Sturmann, Laszlo ^c   Sturmann, Judit ^c   White, Russel ^b   Turner, Nils H ^c   Farrington, Chris ^c   Goldfinger, P J ^c  

^a CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^b GEORGIA STATE UNIVERSITY   (United States)

^c Mount Wilson Observatory   (United States)

^d EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^e OBSERVATOIRE DE BORDEAUX   (France)

^f LABORATOIRE D ASTROPHYSIQUE DE BORDEAUX   (France)

^g UNIVERSITAT AUTÒNOMA DE BARCELONA   (Spain)

^h GEOPHYSICAL LABORATORY   (United States)

ⁱ NATIONAL OPTICAL ASTRONOMY OBSERVATORY   (United States)

Author keywords

infrared: stars; planetary systems; stars: fundamental parameters; stars: individual (55 Cnc); stars: late type; techniques: interferometric

Indexed keywords

EID: 80053556106     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/740/1/49     Document Type: Article

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