Characterizing the cool KOIs. III. KOI 961: A small star with large proper motion and three small planets

Astrophysical Journal

Volumn 747, Issue 2, 2012, Pages

  Muirhead, Philip S ^a   Johnson, John Asher ^a,b   Apps, Kevin ^c   Carter, Joshua A ^d   Morton, Timothy D ^a   Fabrycky, Daniel C ^e   Pineda, John Sebastian ^a   Bottom, Michael ^a   Rojas Ayala, Bárbara ^f   Schlawin, Everett ^g   Hamren, Katherine ^e   Covey, Kevin R ^g   Crepp, Justin R ^a   Stassun, Keivan G ^h,i,j   Pepper, Joshua ^h   Hebb, Leslie ^h   Kirby, Evan N ^a   Howard, Andrew W ^k   Isaacson, Howard T ^k   Marcy, Geoffrey W ^k   Levitan, David ^a   Diaz Santos, Tanio ^l   Armus, Lee ^l   Lloyd, James P ^g   more..

^a CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^b NASA HEADQUARTERS   (United States)

^c Harvard Smithsonian Center for Astrophysics ^*  (United Kingdom)

^d HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^e Santa Cruz   (United States)

^f DIVISION OF INVERTEBRATE ZOOLOGY   (United States)

^g Department of Molecular Biology and Genetics   (United States)

^h VANDERBILT UNIVERSITY   (United States)

ⁱ FISK UNIVERSITY   (United States)

^j MASSACHUSETTS INSTITUTE OF TECHNOLOGY   (United States)

^k UNIVERSITY OF CALIFORNIA   (United States)

^l CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

more..

Author keywords

planetary systems; stars: fundamental parameters; stars: individual (Barnard's Star, KOI 961); stars: late type; stars: low mass

Indexed keywords

EID: 84859726936     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/747/2/144     Document Type: Article

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