Near-term detectability of terrestrial extrasolar planets: TEP network observations of CM Draconis

Astronomy and Astrophysics

Volumn 338, Issue 2, 1998, Pages 479-490

  Deeg, H J ^a   Doyle, L R ^b   Kozhevnikov, V P ^c   Martin E L ^a,j   Oetiker, B ^d   Palaiologou, E ^e   Schneider, J ^f   Afonso, C ^f   Dunham, E W ^g   Jenkins, J M ^b   Ninkov, Z ^h   Stone, R P S ⁱ   Zakharova, P E ^c  

^a INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^b NASA AMES RESEARCH CENTER   (United States)

^c URAL FEDERAL UNIVERSITY   (Russian Federation)

^d UNIVERSITY OF NEW MEXICO   (United States)

^e UNIVERSITY OF CRETE   (Greece)

^f OBSERVATOIRE DE PARIS   (France)

^g LOWELL OBSERVATORY   (United States)

^h ROCHESTER INSTITUTE OF TECHNOLOGY   (United States)

ⁱ UNIVERSITY OF CALIFORNIA   (United States)

^j UNIVERSITY OF CALIFORNIA   (United States)

more..

Author keywords

Binaries: eclipsing; Planetary systems; Stars: flare; Stars: individual: CM Dra; Stars: low mass, brown dwarfs; Techniques: photometric

Indexed keywords

EID: 0000911992     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article

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