Constraining the orbit of the possible companion to Β pictoris

Astronomy and Astrophysics

Volumn 506, Issue 2, 2009, Pages 927-934

  Lagrange, A M ^a   Kasper, M ^b   Boccaletti, A ^c   Chauvin, G ^a   Gratadour, D ^c   Fusco, T ^d   Ehrenreich, D ^a   Apai, D ^e   Mouillet, D ^a   Rouan, D ^c  

^a UNIV GRENOBLE ALPES   (France)

^b EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^c OBSERVATOIRE DE PARIS   (France)

^d ONERA   (France)

^e AURA for the European Space Agency   (United States)

Author keywords

Instrumentation: adaptive optics; Stars: early type; Stars: individual: pictoris; Stars: planetary systems

Indexed keywords

BACKGROUND OBJECTS; FOUR-QUADRANT PHASE MASKS; INSTRUMENTATION: ADAPTIVE OPTICS; NON-DETECTION; ORBITAL MOTIONS; PHYSICAL SEPARATION; PICTORIS; PLANETARY MASS; STARS: EARLY-TYPE; STARS: PLANETARY SYSTEMS; VERY LARGE TELESCOPE;

INSTRUMENTS; MASKS; OPTICAL TELESCOPES; ORBITS; SODIUM COMPOUNDS;

STARS;

EID: 70350459175     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200912098     Document Type: Article

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