Binaries: visual; Techniques: high angular resolution; Binaries:visual; Condition; Exo-planets; Field of views; High contrast imaging; Literature data; Stellar system; Stellars; Techniques: high angular resolutions; Young stars; Astronomy and Astrophysics; Space and Planetary Science; astro-ph.SR; astro-ph.EP
Abstract :
[en] We present the multiple stellar systems observed within the SpHere INfrared survey for Exoplanet (SHINE). SHINE searched for sub-stellar companions to young stars using high contrast imaging. Although stars with known stellar companions within the SPHERE field of view (< 5.5 arcsec) were removed from the original target list, we detected additional stellar companions to 78 of the 463 SHINE targets observed so far. Twenty-seven per cent of the systems have three or more components. Given the heterogeneity of the sample in terms of observing conditions and strategy, tailored routines were used for data reduction and analysis, some of which were specifically designed for these datasets. We then combined SPHERE data with literature and archival data, TESS light curves, and Gaia parallaxes and proper motions for an accurate characterisation of the systems. Combining all data, we were able to constrain the orbits of 25 systems. We carefully assessed the completeness of our sample for separations between 50- 500 mas (corresponding to periods of a few years to a few decades), taking into account the initial selection biases and recovering part of the systems excluded from the original list due to their multiplicity. This allowed us to compare the binary frequency for our sample with previous studies and highlight interesting trends in the mass ratio and period distribution. We also found that, when such an estimate was possible, the values of the masses derived from dynamical arguments were in good agreement with the model predictions. Stellar and orbital spins appear fairly well aligned for the 12 stars that have enough data, which favours a disk fragmentation origin. Our results highlight the importance of combining different techniques when tackling complex problems such as the formation of binaries and show how large samples can be useful for more than one purpose.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Bonavita, M. ; Inaf, Osservatorio Astronomico Di Padova, Padova, Italy ; Scottish Universities Physics Alliance (SUPA), Institute For Astronomy, University Of Edinburgh, Edinburgh, United Kingdom ; Institute For Astronomy, University Of Edinburgh, Edinburgh, United Kingdom
Gratton, R.; Inaf, Osservatorio Astronomico Di Padova, Padova, Italy
Desidera, S.; Inaf, Osservatorio Astronomico Di Padova, Padova, Italy
Squicciarini, V.; Inaf, Osservatorio Astronomico Di Padova, Padova, Italy ; Universitá Degli Studi Di Padova, Dipartimento Di Fisica Ed Astronomia - Galileo Galilei, Padova, Italy
D'Orazi, V.; Inaf, Osservatorio Astronomico Di Padova, Padova, Italy
Zurlo, A.; Núcleo De Astronomía, Facultad De Ingeniería Y Ciencias, Universidad Diego Portales, Santiago, Chile ; Escuela De Ingeniería Industrial, Facultad De Ingeniería Y Ciencias, Universidad Diego Portales, Santiago, Chile ; Aix Marseille Univ, Cnrs, Cnes, Lam, Marseille, France
Biller, B.; Scottish Universities Physics Alliance (SUPA), Institute For Astronomy, University Of Edinburgh, Edinburgh, United Kingdom ; Institute For Astronomy, University Of Edinburgh, Edinburgh, United Kingdom ; Max Planck Institute For Astronomy, Heidelberg, Germany
Chauvin, G.; Univ. Grenoble Alpes, Cnrs, Ipag, Grenoble, France ; Unidad Mixta Internacional Franco-Chilena De Astronomía, CNRS/INSU Umi 3386, Departamento De Astronomía, Universidad De Chile, Santiago, Chile
Fontanive, C.; Inaf, Osservatorio Astronomico Di Padova, Padova, Italy ; Center For Space And Habitability, University Of Bern, Bern, Switzerland
Janson, M.; Max Planck Institute For Astronomy, Heidelberg, Germany ; Department Of Astronomy, Stockholm University, Stockholm, Sweden
Messina, S.; Inaf - Catania Astrophysical Observatory, Catania, Italy
Menard, F.; Univ. Grenoble Alpes, Cnrs, Ipag, Grenoble, France
Meyer, M.; Department Of Astronomy, University Of Michigan, Ann Arbor, United States ; Institute For Particle Physics And Astrophysics, Eth Zurich, Zurich, Switzerland
Vigan, A.; Aix Marseille Univ, Cnrs, Cnes, Lam, Marseille, France
Avenhaus, H.; Institute For Particle Physics And Astrophysics, Eth Zurich, Zurich, Switzerland
Asensio Torres, R.; Max Planck Institute For Astronomy, Heidelberg, Germany
Beuzit, J.-L.; Aix Marseille Univ, Cnrs, Cnes, Lam, Marseille, France ; Univ. Grenoble Alpes, Cnrs, Ipag, Grenoble, France
Boccaletti, A.; Lesia, Observatoire De Paris, Université Psl, Université De Paris, Cnrs, Sorbonne Université, Meudon, France
Bonnefoy, M.; Univ. Grenoble Alpes, Cnrs, Ipag, Grenoble, France
Brandner, W.; Max Planck Institute For Astronomy, Heidelberg, Germany
Cantalloube, F.; Max Planck Institute For Astronomy, Heidelberg, Germany
Cheetham, A.; Geneva Observatory, University Of Geneva, Versoix, Switzerland
Cudel, M.; Univ. Grenoble Alpes, Cnrs, Ipag, Grenoble, France
Daemgen, S.; Institute For Particle Physics And Astrophysics, Eth Zurich, Zurich, Switzerland
Delorme, P.; Univ. Grenoble Alpes, Cnrs, Ipag, Grenoble, France
Desgrange, C.; Núcleo De Astronomía, Facultad De Ingeniería Y Ciencias, Universidad Diego Portales, Santiago, Chile ; Cral, Cnrs, Université Lyon 1, Université De Lyon, Ens, Saint Genis Laval, France
Dominik, C.; Anton Pannekoek Institute For Astronomy, Amsterdam, Netherlands
Engler, N.; Institute For Particle Physics And Astrophysics, Eth Zurich, Zurich, Switzerland
Feautrier, P.; Univ. Grenoble Alpes, Cnrs, Ipag, Grenoble, France
Feldt, M.; Max Planck Institute For Astronomy, Heidelberg, Germany
Galicher, R.; Lesia, Observatoire De Paris, Université Psl, Université De Paris, Cnrs, Sorbonne Université, Meudon, France
Garufi, A.; Institute For Particle Physics And Astrophysics, Eth Zurich, Zurich, Switzerland ; European Space Agency (ESA), Esa Office, Space Telescope Science Institute, Baltimore, United States
Girard, J.; European Southern Observatory, Alonso De Còrdova 3107, Vitacura, Casilla, Santiago, Chile
Grandjean, A.; Univ. Grenoble Alpes, Cnrs, Ipag, Grenoble, France
Hagelberg, J.; Geneva Observatory, University Of Geneva, Versoix, Switzerland
Henning, T.; Max Planck Institute For Astronomy, Heidelberg, Germany
Hunziker, S.; Institute For Particle Physics And Astrophysics, Eth Zurich, Zurich, Switzerland
Kasper, M.; European Southern Observatory (ESO), Garching, Germany
Keppler, M.; Aix Marseille Univ, Cnrs, Cnes, Lam, Marseille, France
Lagadec, E.; Université Côte d'Azur, Oca, Cnrs, Lagrange, France
Lagrange, A.-M.; Univ. Grenoble Alpes, Cnrs, Ipag, Grenoble, France
Langlois, M.; Aix Marseille Univ, Cnrs, Cnes, Lam, Marseille, France ; Cral, Cnrs, Université Lyon 1, Université De Lyon, Ens, Saint Genis Laval, France
Lannier, J.; Univ. Grenoble Alpes, Cnrs, Ipag, Grenoble, France
Lazzoni, C.; Inaf, Osservatorio Astronomico Di Padova, Padova, Italy ; Universitá Degli Studi Di Padova, Dipartimento Di Fisica Ed Astronomia - Galileo Galilei, Padova, Italy
Le Coroller, H.; Aix Marseille Univ, Cnrs, Cnes, Lam, Marseille, France
Ligi, R.; Inaf - Osservatorio Astronomico Di Brera, Merate, Italy
Lombart, M.; Unidad Mixta Internacional Franco-Chilena De Astronomía, CNRS/INSU Umi 3386, Departamento De Astronomía, Universidad De Chile, Santiago, Chile ; Cral, Cnrs, Université Lyon 1, Université De Lyon, Ens, Saint Genis Laval, France
Maire, Anne-Lise ; Université de Liège - ULiège > Unités de recherche interfacultaires > Space sciences, Technologies and Astrophysics Research (STAR)
Mazevet, S.; Inaf - Osservatorio Astrofisico Di Arcetri, Florence, Italy
Mesa, D.; Inaf, Osservatorio Astronomico Di Padova, Padova, Italy
Mouillet, D.; Univ. Grenoble Alpes, Cnrs, Ipag, Grenoble, France
Moutou, C.; Aix Marseille Univ, Cnrs, Cnes, Lam, Marseille, France ; Univ. De Toulouse, Cnrs, Irap, Toulouse, France
Müller, A.; Max Planck Institute For Astronomy, Heidelberg, Germany
Peretti, S.; Geneva Observatory, University Of Geneva, Versoix, Switzerland
Perrot, C.; Lesia, Observatoire De Paris, Université Psl, Université De Paris, Cnrs, Sorbonne Université, Meudon, France ; Space Telescope Science Institute, Baltimore, United States ; Instituto De Física Y Astronomía, Facultad De Ciencias, Universidad De Valparaíso, Valparaíso, Chile
Petrus, S.; Univ. Grenoble Alpes, Cnrs, Ipag, Grenoble, France
Potier, A.; Lesia, Observatoire De Paris, Université Psl, Université De Paris, Cnrs, Sorbonne Université, Meudon, France
Ramos, J.; Max Planck Institute For Astronomy, Heidelberg, Germany
Rickman, E.; NOVA/UVA, Northern, United States
Rouan, D.; Univ. Grenoble Alpes, Cnrs, Ipag, Grenoble, France
Salter, G.; Aix Marseille Univ, Cnrs, Cnes, Lam, Marseille, France
Samland, M.; Max Planck Institute For Astronomy, Heidelberg, Germany ; Department Of Astronomy, Stockholm University, Stockholm, Sweden
Schmidt, T.; Lesia, Observatoire De Paris, Université Psl, Université De Paris, Cnrs, Sorbonne Université, Meudon, France
Sissa, E.; Inaf, Osservatorio Astronomico Di Padova, Padova, Italy
Stolker, T.; Anton Pannekoek Institute For Astronomy, Amsterdam, Netherlands
Szulágyi, J.; Institute For Particle Physics And Astrophysics, Eth Zurich, Zurich, Switzerland
Turatto, M.; Inaf, Osservatorio Astronomico Di Padova, Padova, Italy
Udry, S.; Geneva Observatory, University Of Geneva, Versoix, Switzerland
Wildi, F.; Geneva Observatory, University Of Geneva, Versoix, Switzerland
ERC - European Research Council [BE] FONDECYT - Chile Fondo Nacional de Desarrollo Científico y Tecnológico [CL]
Funding text :
Acknowledgements. The authors would like to thank the referee, Dr. Tokovinin, for providing very insightful feedback that significantly improved the clarity of the paper. SPHERE is an instrument designed and built by a consortium consisting of IPAG (Grenoble, France), MPIA (Heidelberg, Germany), LAM (Marseille, France), LESIA (Paris, France), Laboratoire Lagrange (Nice, France), INAF – Osservatorio di Padova (Italy), Observatoire de Genève (Switzerland), ETH Zürich (Switzerland), NOVA (Netherlands), ONERA (France) and ASTRON (Netherlands) in collaboration with ESO. SPHERE was funded by ESO, with additional contributions from CNRS (France), MPIA (Germany), INAF (Italy), FINES (Switzerland) and NOVA (Netherlands). SPHERE also received funding from the European Commission Sixth and Seventh Framework Programmes as part of the Optical Infrared Coordination Network for Astronomy (OPTICON) under grant number RII3-Ct-2004-001566 for FP6 (2004–2008), grant number 226604 for FP7 (2009–2012) and grant number 312430 for FP7 (2013– 2016). This research has made use of the SIMBAD database and Vizier services, operated at CDS, Strasbourg, France and of the Washington Double Star Catalog maintained at the U.S. Naval Observatory. This work has made use of data from the European Space Agency (ESA) mission Gaia (https://www. cosmos.esa.int/gaia), processed by the Gaia Data Processing and Analysis Consortium (DPAC, https://www.cosmos.esa.int/web/gaia/dpac/ consortium). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement. This paper includes data collected with the TESS mission, obtained from the MAST data archive at the Space Telescope Science Institute (STScI). Funding for the TESS mission is provided by the NASA Explorer Program. STScI is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5–26555. This paper has made use of data products available in ESO archive. This work has been supported by the project PRIN INAF 2016 The Craddle of Life – GENESIS-SKA (General Conditions in Early Planetary Systems for the rise of life with SKA), by the “Progetti Premiali” funding scheme of the Italian Ministry of Education, University, and Research and by the ASI-INAF agreement n.2018-16-HH.0. MB acknowledges funding by the UK Science and Technology Facilities Council (STFC) grant no. ST/M001229/1. AV acknowledges funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement No. 757561). CP acknowledge financial support from Fondecyt (grant 3190691) and financial support from the ICM (Iniciativa Científica Milenio) via the Núcleo Milenio de Formación Planetaria grant, from the Universidad de Val-paraíso.
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