Extrasolar planet detection by binary stellar eclipse timing: Evidence for a third body around CM Draconis

Astronomy and Astrophysics

Volumn 480, Issue 2, 2008, Pages 563-571

  Deeg, J ^a   Ocana B ^a,b   Kozhevnikov, P ^c   Charbonneau, D ^d   O'Donovan, T ^e   Doyle, R ^f  

^a INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^b Institute de Radioastronomie Millimétrique IRAM Núcleo Central   (Spain)

^c URAL FEDERAL UNIVERSITY   (Russian Federation)

^d HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^e CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^f SETI INSTITUTE   (United States)

Author keywords

Eclipses; Stars: binaries: eclipsing; Stars: individual: CM Dra; Stars: planetary systems

Indexed keywords

MOTION CONTROL; SOLAR SYSTEM; SOLAR WIND; STATISTICAL METHODS;

ECLIPSES; STARS: BINARIES: ECLIPSING; STARS: INDIVIDUAL: CM DRA; STARS: PLANETARY SYSTEMS;

PLANETS;

EID: 41449096210     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20079000     Document Type: Article

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