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Dynamical masses of M-dwarf binaries in young moving groups: I. The case of TWA 22 and GJ 2060
Indexado
WoS WOS:000446750800001
Scopus SCOPUS_ID:85054952645
DOI 10.1051/0004-6361/201832924
Año 2018
Tipo artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras


Abstract



Conclusions. TWA22 validates the predictions of recent evolutionary tracks at similar to 20 Myr. On the other hand, we evidence a 1-2 sigma mismatch between the predicted and observed mass of GJ 2060 AB. This slight departure may indicate that one of the stars hosts a tight companion. Alternatively, this would confirm the model's tendency to underestimate the mass of young low-mass stars.

Revista



Revista ISSN
Astronomy & Astrophysics 0004-6361

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Disciplinas de Investigación



WOS
Astronomy & Astrophysics
Scopus
Sin Disciplinas
SciELO
Sin Disciplinas

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Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional



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Autores - Afiliación



Ord. Autor Género Institución - País
1 Rodet, L. Mujer Univ Grenoble Alpes - Francia
Universite Grenoble Alpes - Francia
2 Bonnefoy, M. Hombre Univ Grenoble Alpes - Francia
Universite Grenoble Alpes - Francia
3 Durkan, S. Hombre Queens Univ Belfast - Reino Unido
Stockholm Univ - Suecia
Queen's University Belfast - Reino Unido
Stockholms universitet - Suecia
4 Beust, H. Hombre Univ Grenoble Alpes - Francia
Universite Grenoble Alpes - Francia
5 Lagrange, A. -m. Mujer Univ Grenoble Alpes - Francia
Universite Grenoble Alpes - Francia
6 De Leon, Jerome P. Hombre NASA - Estados Unidos
Max Planck Inst Astron - Alemania
NASA Goddard Space Flight Center - Estados Unidos
Max Planck Institute for Astronomy - Alemania
7 Janson, M. Hombre Stockholm Univ - Suecia
Stockholms universitet - Suecia
8 Grandjean, Antoine Hombre Univ Grenoble Alpes - Francia
Universite Grenoble Alpes - Francia
9 Chauvin, Gael Hombre Univ Grenoble Alpes - Francia
Universidad de Chile - Chile
Universite Grenoble Alpes - Francia
10 Messina, Sergio Hombre Istituto Nazionale di Astrofisica - Italia
Osservatorio Astronomico di Padova - Italia
11 Maire, A. -L. Mujer Max Planck Inst Astron - Alemania
Max Planck Institute for Astronomy - Alemania
12 Brandner, W. Hombre Max Planck Inst Astron - Alemania
Max Planck Institute for Astronomy - Alemania
13 Girard, J. H. Hombre Univ Grenoble Alpes - Francia
ESO - Chile
Universite Grenoble Alpes - Francia
European Southern Observatory Santiago - Chile
14 Delorme, P. Hombre Univ Grenoble Alpes - Francia
Universite Grenoble Alpes - Francia
15 Biller, Beth Mujer UNIV EDINBURGH - Reino Unido
University of Edinburgh, Institute for Astronomy - Reino Unido
16 Bergfors, C. - Max Planck Inst Astron - Alemania
UCL - Reino Unido
Max Planck Institute for Astronomy - Alemania
University College London - Reino Unido
17 Lacour, S. Hombre UNIV PARIS 06 - Francia
LESIA - Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique - Francia
Sorbonne Université - Francia
18 Feldt, M. Hombre Max Planck Inst Astron - Alemania
Max Planck Institute for Astronomy - Alemania
19 Henning, Thomas Hombre Max Planck Inst Astron - Alemania
Max Planck Institute for Astronomy - Alemania
20 Boccaletti, A. Hombre UNIV PARIS 06 - Francia
LESIA - Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique - Francia
Sorbonne Université - Francia
21 MORALES-PERALTA, JUAN CARLOS Hombre Univ Grenoble Alpes - Francia
Universite Grenoble Alpes - Francia
22 Berger, J. P. - Universite Grenoble Alpes - Francia
22 Berger, Jean-Philippe Hombre Univ Grenoble Alpes - Francia
Universite Grenoble Alpes - Francia
23 Monin, Jean-Louis Hombre Univ Grenoble Alpes - Francia
Universite Grenoble Alpes - Francia
24 Celino, J. J. Hombre Université de Genève - Suiza
Faculty of Science - Suiza
25 Peretti, Sebastien Hombre Univ Geneva - Suiza
Université de Genève - Suiza
Faculty of Science - Suiza
26 Ségransan, Damien Hombre Univ Geneva - Suiza
Université de Genève - Suiza
Faculty of Science - Suiza
27 Allard, F. Mujer Univ Lyon - Francia
Ecole Normale Supérieure de Lyon - Francia
28 Homeier, D. Hombre Heidelberg Univ - Alemania
Landessternwarte Heidelberg - Alemania
29 Vigan, Arthur Hombre Aix Marseille Univ - Francia
Laboratoire d'Astrophysique de Marseille - Francia
30 La Nglois, M. Mujer Univ Lyon - Francia
Aix Marseille Univ - Francia
Max Planck Inst Astron - Alemania
Ecole Normale Supérieure de Lyon - Francia
Laboratoire d'Astrophysique de Marseille - Francia
Max Planck Institute for Astronomy - Alemania
31 Hagelberg, J. Mujer Univ Grenoble Alpes - Francia
Universite Grenoble Alpes - Francia
32 Menard, Francois Hombre Univ Grenoble Alpes - Francia
Universite Grenoble Alpes - Francia
33 Ahumada, Danay Mujer Swiss Fed Inst Technol - Suiza
ETH Zurich - Suiza
34 Beuzit, J. -L. Hombre Univ Grenoble Alpes - Francia
Universite Grenoble Alpes - Francia
35 Delboulbe, Alain Hombre Univ Grenoble Alpes - Francia
Universite Grenoble Alpes - Francia
36 Desidera, S. Hombre Osservatorio Astronomico di Padova - Italia
37 Gratton, Raffaele Hombre Istituto Nazionale di Astrofisica - Italia
Osservatorio Astronomico di Padova - Italia
38 Lannier, J. Mujer Univ Grenoble Alpes - Francia
Universite Grenoble Alpes - Francia
39 Ligi, Roxanne Mujer Aix Marseille Univ - Francia
Laboratoire d'Astrophysique de Marseille - Francia
40 Maurel, D. - Univ Grenoble Alpes - Francia
Universite Grenoble Alpes - Francia
41 Mesa, Dino Hombre Istituto Nazionale di Astrofisica - Italia
Osservatorio Astronomico di Padova - Italia
42 Merschmeyer, M. Hombre Swiss Fed Inst Technol - Suiza
ETH Zurich - Suiza
43 Pavlov, Alexey Hombre Max Planck Inst Astron - Alemania
Max Planck Institute for Astronomy - Alemania
44 FERNANDEZ-FERNANDEZ, MARIO ALBERTO Hombre Max Planck Inst Astron - Alemania
Max Planck Institute for Astronomy - Alemania
45 Rigal, R. - Anton Pannekoek Inst Astron - Países Bajos
Anton Pannekoek Institute for Astronomy - Países Bajos
Anton Pannekoek Instituut voor Sterrenkunde - Países Bajos
46 Roelfsema, R. Hombre NOVA Opt Infrared Instrumentat Grp - Países Bajos
NOVA Optical Infrared Instrumentation Group - Países Bajos
47 Salter, Graeme Hombre Aix Marseille Univ - Francia
Laboratoire d'Astrophysique de Marseille - Francia
48 La Nglois, M. Mujer Univ Lyon - Francia
Aix Marseille Univ - Francia
Max Planck Inst Astron - Alemania
Ecole Normale Supérieure de Lyon - Francia
Laboratoire d'Astrophysique de Marseille - Francia
Max Planck Institute for Astronomy - Alemania
49 Schmidt, T. - UNIV PARIS 06 - Francia
50 Stadler, E. - Univ Grenoble Alpes - Francia
Universite Grenoble Alpes - Francia
51 Weber, Luc - Université de Genève - Suiza
Faculty of Science - Suiza

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Financiamiento



Fuente
European Commission
CNRS
ESO
Swiss National Science Foundation (SNSF)
STFC
Seventh Framework Programme
CNRS (France)
MPIA (Germany)
INAF (Italy)
FINES (Switzerland)
NOVA (Netherlands)
Agence Nationale de la Recherche
SNSF
Programme National de Planetologie (PNP)
French Labex OSUG@2020 (Investissements d'avenir)
Programme National de Physique Stellaire (PNPS) of CNRS-INSU in France
Programme National de Planetologie (PNP, INSU)
Programme National de Physique Stellaire (PNPS, INSU)
OSUG@2020 labex
Rhone-Alpes region
Agence Nationale de la Recherche (GIPSE)
Equip@Meso project of the programme Investissements d'Avenir

Muestra la fuente de financiamiento declarada en la publicación.

Agradecimientos



Agradecimiento
We thank Carine Babusiaux, Benjamin Montet, and Thierry Forveille for fruitful discussions, as well as the anonymous referee for reviewing our work and for insightful and constructive comments which improved the manuscript. The project is supported by CNRS, by the Agence Nationale de la Recherche (ANR-14-CE33-0018, GIPSE), the OSUG@2020 Labex, and the Programme National de Planetologie (PNP, INSU) and Programme National de Physique Stellaire (PNPS, INSU). Most of the computations presented in this paper were performed using the Froggy platform of the CIMENT infrastructure (https://ciment.ujf-grenoble.fr), which is supported by the Rhone-Alpes region (GRANT CPER07_13 CIRA), the OSUG@2020 Labex (reference ANR10 LABX56), and the Equip@Meso project (reference ANR-10-EQPX-29-01) of the programme Investissements d'Avenir, supervised by the Agence Nationale pour la Recherche. This research has made use of the SIMBAD database operated at the CDS (Strasbourg, France). Research on moving groups by Thomas Henning is supported by the DFG-SFB 881 "The Milky Way System." 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 Genave (Switzerland), ETH Zurich (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). We also acknowledge financial support from the Programme National de Planetologie (PNP) and the Programme National de Physique Stellaire (PNPS) of CNRS-INSU in France. This work has also been supported by a grant from the French Labex OSUG@2020 (Investissements d'avenir - ANR10 LABX56). The project is supported by CNRS, by the Agence Nationale de la Recherche (ANR-14-CE33-0018). It has also been carried out within the frame of the National Centre for Competence in Research PlanetS supported by the Swiss National Science Foundation (SNSF). MRM, HMS, and SD are pleased to acknowledge the financial support of the SNSF. Finally, this work has made use of the the SPHERE Data Centre, jointly operated by OSUG/IPAG (Grenoble), PYTHEAS/LAM/CESAM (Marseille), OCA/Lagrange (Nice), and Observatoire de Paris/LESIA (Paris). We thank P. Delorme and E. Lagadec (SPHERE Data Centre) for their efficient help during the data reduction process.

Muestra la fuente de financiamiento declarada en la publicación.