A survey of young, nearby, and dusty stars conducted to understand the formation of wide-orbit giant planets
Year: 2013
Type: article
Abstract: Context. Over the past decade, direct imaging has confirmed the existence of substellar companions on wide orbits from their parent stars. To understand the formation and evolution mechanisms of these companions, their individual as well as the full population properties must be characterized.
Source: Astronomy and Astrophysics
Institutions: Centre National de la Recherche Scientifique, Université Joseph Fourier, Institut de Planétologie et d'Astrophysique de Grenoble, Max Planck Institute for Astronomy, University of Toronto, Osservatorio Astronomico di Padova, National Institute for Astrophysics, European Southern Observatory
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: bronze
OpenAlex ID: W1597385910
