Article (Scientific journals)
Dynamical masses for two M1 + mid-M dwarf binaries monitored during the SPHERE-SHINE survey
Biller, Beth A.; Grandjean, Antoine; Messina, Sergio et al.
2022In Astronomy and Astrophysics, 658, p. 145
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Keywords :
Astrometry; Binaries: visual; Infrared: stars; Stars: fundamental parameters; Stars: imaging; Stars: low-mass; Binaries:visual; Direct imaging; Dwarf binaries; HIPPARCOS; Infrared: star; Radial velocity; Stars: low mass; Stars:fundamental parameters; Stars:imaging; Astronomy and Astrophysics; Space and Planetary Science; astro-ph.SR
Abstract :
[en] We present orbital fits and dynamical masses for HIP 113201AB and HIP 36985AB, two M1 + mid-M dwarf binary systems monitored as part of the SPHERE-SHINE survey. To robustly determine the age of both systems via gyrochronology, we undertook a photometric monitoring campaign for HIP 113201 and GJ 282AB, the two wide K star companions to HIP 36985, using the 40 cm Remote Observatory Atacama Desert telescope. Based on this monitoring and gyrochronological relationships, we adopt ages of 1.2 ± 0.1 Gyr for HIP 113201AB and 750 ± 100 Myr for HIP 36985AB. These systems are sufficiently old that we expect that all components of these binaries have reached the main sequence. To derive dynamical masses for all components of the HIP 113201AB and HIP 36985AB systems, we used parallel-tempering Markov chain Monte Carlo sampling to fit a combination of radial velocity, direct imaging, and Gaia and HIPPARCOS astrometry. Fitting the direct imaging and radial velocity data for HIP 113201 yields a primary mass of 0.54 ± 0.03 M⊙, fully consistent with its M1 spectral type, and a secondary mass of 0.145 ± M⊙. The secondary masses derived with and without including HIPPARCOS-Gaia data are all considerably more massive than the 0.1 M⊙ mass estimated from the photometry of the companion. Thus, the dynamical impacts of this companion suggest that it is more massive than expected from its photometry. An undetected brown dwarf companion to HIP 113201B could be a natural explanation for this apparent discrepancy. At an age >1 Gyr, a 30 MJup companion to HIP 113201B would make a negligible (<1%) contribution to the system luminosity but could have strong dynamical impacts. Fitting the direct imaging, radial velocity, and HIPPARCOS-Gaia proper motion anomaly for HIP 36985AB, we find a primary mass of 0.54 ± 0.01 M⊙ and a secondary mass of 0.185 ± 0.001 M⊙, which agree well with photometric estimates of component masses, the masses estimated from MK- mass relationships for M dwarf stars, and previous dynamical masses in the literature.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Biller, Beth A.;  SUPA, Institute for Astronomy, University of Edinburgh, Edinburgh, United Kingdom ; Centre for Exoplanet Science, University of Edinburgh, Edinburgh, United Kingdom ; Max Planck Institute for Astronomy, Heidelberg, Germany
Grandjean, Antoine;  Univ. Grenoble Alpes, CNRS, IPAG, Grenoble, France
Messina, Sergio ;  INAF - Catania Astrophysical Observatory, Catania, Italy
Desidera, Silvano ;  INAF - Osservatorio Astronomico di Padova, Padova, Italy
Delorme, Philippe;  Univ. Grenoble Alpes, CNRS, IPAG, Grenoble, France
Lagrange, Anne-Marie ;  Univ. Grenoble Alpes, CNRS, IPAG, Grenoble, France ; LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de Paris, Meudon, France ; IMCCE - Observatoire de Paris, Paris, France
Hambsch, Franz-Josef;  American Association of Variable Star Observers (AAVSO), Cambridge, United States ; Vereniging voor Sterrenkunde (VVS), Brugge, Belgium
Mesa, Dino ;  INAF - Osservatorio Astronomico di Padova, Padova, Italy
Janson, Markus ;  Max Planck Institute for Astronomy, Heidelberg, Germany ; Institutionen för Astronomi, Stockholms Universitet, Stockholm, Sweden
Gratton, Raffaele ;  INAF - Osservatorio Astronomico di Padova, Padova, Italy
D'Orazi, Valentina ;  INAF - Osservatorio Astronomico di Padova, Padova, Italy
Langlois, Maud ;  CRAL, UMR 5574, CNRS, Université de Lyon, ENS, France ; Aix Marseille Univ, CNRS, CNES, LAM, Marseille, France
Maire, Anne-Lise ;  Université de Liège - ULiège > Unités de recherche interfacultaires > Space sciences, Technologies and Astrophysics Research (STAR) ; Max Planck Institute for Astronomy, Heidelberg, Germany
Schlieder, Joshua;  Max Planck Institute for Astronomy, Heidelberg, Germany ; Exoplanets and Stellar Astrophysics Laboratory, NASA Goddard Space Flight Center, Greenbelt, United States
Henning, Thomas;  Max Planck Institute for Astronomy, Heidelberg, Germany
Zurlo, Alice;  Aix Marseille Univ, CNRS, CNES, LAM, Marseille, France ; Núcleo de Astronomiá, Facultad de Ingenieriá y Ciencias, Universidad Diego Portales, Santiago, Chile ; Escuela de Ingenieriá Industrial, Facultad de Ingenieriá y Ciencias, Universidad Diego Portales, Santiago, Chile
Hagelberg, Janis ;  Geneva Observatory, University of Geneva, Versoix, Switzerland
Brown-Sevilla, S. ;  Max Planck Institute for Astronomy, Heidelberg, Germany
Romero, C.;  Univ. Grenoble Alpes, CNRS, IPAG, Grenoble, France ; ESO Vitacura, Alonso de Córdova 3107, Santiago de Chile, Chile
Bonnefoy, Mickaël;  Univ. Grenoble Alpes, CNRS, IPAG, Grenoble, France
Chauvin, Gael ;  Univ. Grenoble Alpes, CNRS, IPAG, Grenoble, France ; Unidad Mixta Internacional Franco-Chilena de Astronomiá, CNRS/INSU UMI 3386, Departamento de Astronomiá, Universidad de Chile, Santiago, Chile
Feldt, Markus;  Max Planck Institute for Astronomy, Heidelberg, Germany
Meyer, Michael;  Department of Astronomy, University of Michigan, Ann Arbor, United States ; Institute for Particle Physics and Astrophysics, ETH Zurich, Zurich, Switzerland
Vigan, Arthur ;  Aix Marseille Univ, CNRS, CNES, LAM, Marseille, France
Pavlov, A. ;  Max Planck Institute for Astronomy, Heidelberg, Germany
Soenke, C.;  European Southern Observatory (ESO), Garching, Germany
Lemignant, D.;  Aix Marseille Univ, CNRS, CNES, LAM, Marseille, France
Roux, A.;  Univ. Grenoble Alpes, CNRS, IPAG, Grenoble, France
More authors (18 more) Less
Language :
English
Title :
Dynamical masses for two M1 + mid-M dwarf binaries monitored during the SPHERE-SHINE survey
Publication date :
February 2022
Journal title :
Astronomy and Astrophysics
ISSN :
0004-6361
eISSN :
1432-0746
Publisher :
EDP Sciences
Volume :
658
Pages :
A145
Peer reviewed :
Peer Reviewed verified by ORBi
Funders :
SFTC - Science and Technology Facilities Council [GB]
FONDECYT - Chile Fondo Nacional de Desarrollo Científico y Tecnológico [CL]
Funding text :
B.B. acknowledges funding by the UK Science and Technology Facilities Council (STFC) grant no. ST/M001229/1. B.B. would like to acknowledge valuable conversations with Trent Dupuy and Mariangela Bonavita which improved this manuscript. This work has been supported by the PRININAF 2019 “Planetary systems at young ages (PLATEA)” and the ASI-INAF agreement n.2018-16-HH.0. A.Z. acknowledges support from the FONDECYT Iniciación en investigación project number 11190837. 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 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 Planétologie (PNP) and the Programme National de Physique Stellaire (PNPS) of CNRSINSU 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). M.R.M., H.M.S., and S.D. are pleased to acknowledge this financial support of the SNSF. Finally, this work has made use of the SPHERE Data Centre, jointly operated by OSUG/IPAG (Grenoble), PYTHEAS/LAM/CESAM (Marseille), OCA/Lagrange (Nice), Observatoire de Paris/LESIA (Paris), and Observatoire de Lyon, also supported by a grant from Labex OSUG@2020 (Investissements d’avenir – ANR10 LABX56).We thank P. Delorme and E. Lagadec (SPHERE Data Centre) for their efficient help during the data reduction process.
Commentary :
accepted to A&A
Available on ORBi :
since 06 September 2022

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