Article (Scientific journals)
The EBLM project - IX. Five fully convective M-dwarfs, precisely measured with CHEOPS and TESS light curves
Sebastian, D.; Swayne, M. I.; Maxted, P. F. L. et al.
2022In Monthly Notices of the Royal Astronomical Society
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Keywords :
binaries: eclipsing; stars: fundamental parameters; stars: low-mass; techniques: photometric; techniques: spectroscopic; Astrophysics - Solar; and Stellar Astrophysics; Astrophysics - Earth and Planetary; Astrophysics
Abstract :
[en] Eclipsing binaries are important benchmark objects to test and calibrate stellar structure and evolution models. This is especially true for binaries with a fully convective M-dwarf component for which direct measurements of these stars' masses and radii are difficult using other techniques. Within the potential of M-dwarfs to be exoplanet host stars, the accuracy of theoretical predictions of their radius and effective temperature as a function of their mass is an active topic of discussion. Not only the parameters of transiting exoplanets but also the success of future atmospheric characterisation rely on accurate theoretical predictions. We present the analysis of five eclipsing binaries with low-mass stellar companions out of a sub-sample of 23, for which we obtained ultra high-precision light curves using the CHEOPS satellite. The observation of their primary and secondary eclipses are combined with spectroscopic measurements to precisely model the primary parameters and derive the M-dwarfs mass, radius, surface gravity, and effective temperature estimates using the PYCHEOPS data analysis software. Combining these results to the same set of parameters derived from TESS light curves, we find very good agreement (better than 1% for radius and better than 0.2% for surface gravity). We also analyse the importance of precise orbits from radial velocity measurements and find them to be crucial to derive M-dwarf radii in a regime below 5% accuracy. These results add five valuable data points to the mass-radius diagram of fully-convective M-dwarfs.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Sebastian, D.;  School of Physics, and Astronomy, University of Birmingham, Edgbaston, Birmimgham, B15 2TT, UK
Swayne, M. I.;  Keele University, Department of Physics and Astrophysics
Maxted, P. F. L.;  Keele University, Department of Physics and Astrophysics
Triaud, A. H. M. J.;  School of Physics, and Astronomy, University of Birmingham, Edgbaston, Birmimgham, B15 2TT, UK
Sousa, S. G.;  University of Porto, Center for Astrophysics
Olofsson, G.;  AlbaNova University Center
Beck, M.;  Observatoire Astronomique de l'Université de Genéve, Chemin Pegasi 51, Versoix, Switzerland
Billot, N.;  Observatoire Astronomique de l'Université de Genéve, Chemin Pegasi 51, Versoix, Switzerland
Hoyer, S.;  Aix-Marseille Universite, Laboratoire d'Astrophysique
Gill, S.;  University of Warwick, Department of Physics
Heidari, N.;  Aix-Marseille Universite, Laboratoire d'Astrophysique
Martin, D. V.;  The Ohio State University
Persson, C. M.;  Onsala Space Observatory
Standing, M. R.;  School of Physics, and Astronomy, University of Birmingham, Edgbaston, Birmimgham, B15 2TT, UK
Alibert, Y.;  University of Bern, Physics Institute
Alonso, R.;  Astrophysical Institute of the Canaries, University of La Laguna, Department of Astrophysics
Anglada, G.;  Institut de Ciencies de l'Espai (ICE, CSIC), Campus UAB, Can Magrans s/n, 08193 Bellaterra, Spain, Institut d'Estudis Espacials de Catalunya (IEEC), 08034 Barcelona, Spain
Asquier, J.;  ESTEC, European Space Agency, 2201AZ, Noordwijk, NL
Bárczy, T.;  Admatis, 5. Kandó Kálmán Street, 3534 Miskolc, Hungary
Barrado, D.;  Depto. de Astrofisica, Centro de Astrobiologia (CSIC-INTA), ESAC campus, 28692 Villanueva de la Cañada (Madrid), Spain
Barros, S. C. C.;  University of Porto, Center for Astrophysics, -
Battley, M. P.;  University of Warwick, Department of Physics
Baumjohann, W.;  Austrian Institute of Space Science Research
Beck, T.;  University of Bern, Physics Institute
Benz, W.;  University of Bern, Physics Institute, -
Bergomi, M.;  Astronomical Observatory of Padua
Boisse, I.;  Aix-Marseille Universite, Laboratoire d'Astrophysique
Bonfils, X.;  Institute de Planetologie et d'Astrophysique de Grenoble
Brandeker, A.;  AlbaNova University Center
Broeg, C.;  University of Bern, Physics Institute, -
Cabrera, J.;  Helmholtz Institute for Planetary Research, Berlin
Charnoz, S.;  Institut de Physique du Globe de Paris
Cameron, A. Collier;  Scottish Universities Physics Alliance
Csizmadia, Sz;  Helmholtz Institute for Planetary Research, Berlin
Davies, M. B.;  University of Lund, Sweden
Deleuil, M.;  Aix-Marseille Universite, Laboratoire d'Astrophysique
Delrez, Laetitia  ;  Université de Liège - ULiège > Département d'astrophysique, géophysique et océanographie (AGO) > Exoplanets in Transit: Identification and Characterization
Demangeon, O. D. S.;  University of Porto, Center for Astrophysics, -
Demory, B. -O.;  Center for Space and Habitability, Gesellsschaftstrasse 6, 3012 Bern, Switzerland
Dransfield, G.;  School of Physics, and Astronomy, University of Birmingham, Edgbaston, Birmimgham, B15 2TT, UK
Ehrenreich, D.;  Observatoire Astronomique de l'Université de Genéve, Chemin Pegasi 51, Versoix, Switzerland
Erikson, A.;  Helmholtz Institute for Planetary Research, Berlin
Fortier, A.;  University of Bern, Physics Institute, -
Fossati, L.;  Austrian Institute of Space Science Research
Fridlund, M.;  Leiden Observatory, Onsala Space Observatory
Gandolfi, D.;  University of Turin, Department of Physics
Gillon, Michaël  ;  Université de Liège - ULiège > Département d'astrophysique, géophysique et océanographie (AGO) > Exoplanets in Transit: Identification and Characterization
Güdel, M.;  University of Vienna, Department of Astronomy
Hasiba, J.;  Austrian Institute of Space Science Research
Hébrard, G.;  Institut d'Astrophysique de Paris
Heng, K.;  Center for Space and Habitability, Gesellsschaftstrasse 6, 3012 Bern, Switzerland, Department of Physics, University of Warwick, Gibbet Hill Road, Coventry CV4 7AL, United Kingdom
Isaak, K. G.;  Science and Operations Department - Science Division (SCI-SC), Directorate of Science, European Space Agency (ESA), European Space Research and Technology Centre (ESTEC), Keplerlaan 1, 2201-AZ Noordwijk, The Netherlands
Kiss, L. L.;  Konkoly Observatory, -
Kopp, E.;  Helmholtz Institute for Planetary Research, Berlin
Kunovac, V.;  School of Physics, and Astronomy, University of Birmingham, Edgbaston, Birmimgham, B15 2TT, UK
Laskar, J.;  Observatoire de Paris, Institut de Mecanique Celeste et de Calcul des Ephemerides
des Etangs, A. Lecavelier;  Institut d'Astrophysique de Paris
Lendl, M.;  Observatoire Astronomique de l'Université de Genéve, Chemin Pegasi 51, Versoix, Switzerland
Lovis, C.;  Observatoire Astronomique de l'Université de Genéve, Chemin Pegasi 51, Versoix, Switzerland
Magrin, D.;  Astronomical Observatory of Padua
McCormac, J.;  University of Warwick, Department of Physics
Miller, N. J.;  Keele University, Department of Physics and Astrophysics
Nascimbeni, V.;  Astronomical Observatory of Padua
Ottensamer, R.;  University of Vienna, Department of Astronomy
Pagano, I.;  German Aerospace Center, Berlin
Pallé, E.;  Astrophysical Institute of the Canaries
Pepe, F. A.;  Observatoire Astronomique de l'Université de Genéve, Chemin Pegasi 51, Versoix, Switzerland
Peter, G.;  Astronomical Observatory of Padua
Piotto, G.;  Astronomical Observatory of Padua, -
Pollacco, D.;  University of Warwick, Department of Physics
Queloz, D.;  University of Cambridge, Institute of Astronomy, Technical University of Berlin, Center for Astronomy and Astrophysics
Ragazzoni, R.;  Astronomical Observatory of Padua, -
Rando, N.;  ESTEC, European Space Agency, 2201AZ, Noordwijk, NL
Rauer, H.;  Helmholtz Institute for Planetary Research, Berlin, Free University of Berlin, Department of Geosciences, Eotvos Lorand University, Hungary
Ribas, I.;  Institut de Ciencies de l'Espai (ICE, CSIC), Campus UAB, Can Magrans s/n, 08193 Bellaterra, Spain, Institut d'Estudis Espacials de Catalunya (IEEC), 08034 Barcelona, Spain
Lalitha, S.;  School of Physics, and Astronomy, University of Birmingham, Edgbaston, Birmimgham, B15 2TT, UK
Santerne, A.;  Aix-Marseille Universite, Laboratoire d'Astrophysique
Santos, N. C.;  University of Porto, Center for Astrophysics, -
Scandariato, G.;  German Aerospace Center, Berlin
Ségransan, D.;  Observatoire Astronomique de l'Université de Genéve, Chemin Pegasi 51, Versoix, Switzerland
Simon, A. E.;  University of Bern, Physics Institute
Smith, A. M. S.;  Helmholtz Institute for Planetary Research, Berlin
Steller, M.;  Austrian Institute of Space Science Research
Szabó, Gy M.;  Eotvos Lorand University, Hungary, University of Cambridge, Institute of Astronomy
Thomas, N.;  University of Bern, Physics Institute
Udry, S.;  Observatoire Astronomique de l'Université de Genéve, Chemin Pegasi 51, Versoix, Switzerland
Van Grootel, Valérie  ;  Université de Liège - ULiège > Département d'astrophysique, géophysique et océanographie (AGO) > Astrophysique stellaire théorique et astérosismologie
Walton, N. A.;  Lowell Observatory, Arizona
More authors (78 more) Less
Language :
English
Title :
The EBLM project - IX. Five fully convective M-dwarfs, precisely measured with CHEOPS and TESS light curves
Publication date :
01 September 2022
Journal title :
Monthly Notices of the Royal Astronomical Society
ISSN :
0035-8711
eISSN :
1365-2966
Publisher :
Oxford University Press, Oxford, Gb
Peer reviewed :
Peer Reviewed verified by ORBi
Available on ORBi :
since 29 September 2022

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