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The planet companion around β Pictoris

Published online by Cambridge University Press:  10 November 2011

Anne-Marie Lagrange
Affiliation:
Laboratoire dAstrophysique de Grenoble, France email: [email protected], [email protected], [email protected], [email protected], [email protected]
Mickaël Bonnefoy
Affiliation:
Laboratoire dAstrophysique de Grenoble, France email: [email protected], [email protected], [email protected], [email protected], [email protected]
Gael Chauvin
Affiliation:
Laboratoire dAstrophysique de Grenoble, France email: [email protected], [email protected], [email protected], [email protected], [email protected]
Daniel Apai
Affiliation:
Space Telesope Sciente Institute, 3700 San Martin Dr. Baltimore, MD 21218, USA email: [email protected]
David Ehrenreich
Affiliation:
Laboratoire dAstrophysique de Grenoble, France email: [email protected], [email protected], [email protected], [email protected], [email protected]
Anthony Boccaletti
Affiliation:
LESIA, Observatoire de Paris, place Jules Janssen, 92195 Meudon, France email: [email protected], [email protected], [email protected], [email protected]
Damien Gratadour
Affiliation:
LESIA, Observatoire de Paris, place Jules Janssen, 92195 Meudon, France email: [email protected], [email protected], [email protected], [email protected]
Daniel Rouan
Affiliation:
LESIA, Observatoire de Paris, place Jules Janssen, 92195 Meudon, France email: [email protected], [email protected], [email protected], [email protected]
David Mouillet
Affiliation:
Laboratoire dAstrophysique de Grenoble, France email: [email protected], [email protected], [email protected], [email protected], [email protected]
Sylvestre Lacour
Affiliation:
LESIA, Observatoire de Paris, place Jules Janssen, 92195 Meudon, France email: [email protected], [email protected], [email protected], [email protected]
Markus Kasper
Affiliation:
ESO, Karl Schwarzschild St, 2, 85748 Garching bei Muenchen, Germany email: [email protected]
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Abstract

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The β Pic disk of dust and gas has been regarded as the prototype of young planetary systems since the 1980s and has revealed over the years an impressive amount of indirect signs pointing toward the presence of at least one giant planet. We present here the recently detected first giant planet around this star. We show how this planet could explain some very peculiar features of the star environment (disk, spectroscopic variability), and how it constrains the scenarios of planetary system formation (timescales, mechanisms).

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2011

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