The SOPHIE search for northern extrasolar planets: XVII. A wealth of new objects: Six cool Jupiters, three brown dwarfs, and 16 low-mass binary stars
- Autores
- Dalal, S.; Kiefer, F.; Hébrard, G.; Sahlmann, J.; Sousa, S.G.; Forveille, T.; Delfosse, X.; Arnold, L.; Astudillo Defru, Nicola; Bonfils, X.; Boisse, I.; Bouchy, F.; Bourrier, V.; Brugger, B.; Cortés Zuleta, P.; Deleuil, M.; Demangeon, O. D. S.; Díaz, Rodrigo Fernando; Hara, N. C.; Heidari, N.; Hobson, M. J.; Lopez, T.; Lovis, C.; Martioli, E.; Mignon, L.; Mousis, O.; Moutou, C.; Rey, J.; Santerne, A.; Santos, N. C.; Ségransan, D.; Strøm, P. A.; Udry, S.
- Año de publicación
- 2021
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Distinguishing classes within substellar objects and understanding their formation and evolution need larger samples of substellar companions such as exoplanets, brown dwarfs, and low-mass stars. In this paper, we look for substellar companions using radial velocity surveys of FGK stars with the SOPHIE spectrograph at the Observatoire de Haute-Provence. We assign here the radial velocity variations of 27 stars to their orbital motion induced by low-mass companions. We also constrained their plane-of-the-sky motion using HIPPARCOS and Gaia Data Release 1 measurements, which constrain the true masses of some of these companions. We report the detection and characterization of six cool Jupiters, three brown dwarf candidates, and 16 low-mass stellar companions. We additionally update the orbital parameters of the low-mass star HD 8291 B, and we conclude that the radial velocity variations of HD 204277 are likely due to stellar activity despite resembling the signal of a giant planet. One of the new giant planets, BD+631405 b, adds to the population of highly eccentric cool Jupiters, and it is presently the most massive member. Two of the cool Jupiter systems also exhibit signatures of an additional outer companion. The orbital periods of the new companions span 30 days to 11.5 yr, their masses 0.72 MJ-0.61 Ma, and their eccentricities 0.04-0.88. These discoveries probe the diversity of substellar objects and low-mass stars, which will help constrain the models of their formation and evolution.
Fil: Dalal, S.. Institut d’Astrophysique de Paris; Francia
Fil: Kiefer, F.. Institut d’Astrophysique de Paris; Francia. Centre National de la Recherche Scientifique. Observatoire de Paris; Francia
Fil: Hébrard, G.. Université d’Aix-Marseille; Francia. Institut d’Astrophysique de Paris; Francia
Fil: Sahlmann, J.. European Space Astronomy Centre; España
Fil: Sousa, S.G.. Universidad de Porto; Portugal
Fil: Forveille, T.. Universite Grenoble Alpes; Francia
Fil: Delfosse, X.. Universite Grenoble Alpes; Francia
Fil: Arnold, L.. Université d’Aix-Marseille; Francia
Fil: Astudillo Defru, Nicola. Universidad Católica de la Santísima Concepción; Chile
Fil: Bonfils, X.. Universite Grenoble Alpes; Francia
Fil: Boisse, I.. Université d’Aix-Marseille; Francia
Fil: Bouchy, F.. Universidad de Ginebra; Suiza
Fil: Bourrier, V.. Universidad de Ginebra; Suiza
Fil: Brugger, B.. Université d’Aix-Marseille; Francia
Fil: Cortés Zuleta, P.. Université d’Aix-Marseille; Francia
Fil: Deleuil, M.. Université d’Aix-Marseille; Francia
Fil: Demangeon, O. D. S.. Universidad de Porto; Portugal
Fil: Díaz, Rodrigo Fernando. Consejo Nacional de Investigaciones Científicas y Técnicas. Instituto de Ciencias Físicas. - Universidad Nacional de San Martín. Instituto de Ciencias Físicas; Argentina. Universidad Nacional de San Martín. Escuela de Política y Gobierno; Argentina
Fil: Hara, N. C.. Universidad de Ginebra; Suiza
Fil: Heidari, N.. Universite de Nice-Sophia Antipolis. Laboratoire Joseph-louis Lagrange; Francia. Shahid Beheshti University; Irán. Université d’Aix-Marseille; Francia
Fil: Hobson, M. J.. Pontificia Universidad Católica de Chile; Chile. Instituto Milenio de Astrofísica; Chile
Fil: Lopez, T.. Université d’Aix-Marseille; Francia
Fil: Lovis, C.. Universidad de Ginebra; Suiza
Fil: Martioli, E.. Institut d’Astrophysique de Paris; Francia. Laboratório Nacional de Astrofísica; Brasil
Fil: Mignon, L.. Universidad Católica de la Santísima Concepción; Chile
Fil: Mousis, O.. Université d’Aix-Marseille; Francia
Fil: Moutou, C.. Universite de Toulose - Le Mirail; Francia
Fil: Rey, J.. Carnegie Institution of Washington. Las Campanas Observatory; Chile
Fil: Santerne, A.. Université d’Aix-Marseille; Francia
Fil: Santos, N. C.. Universidad de Porto; Portugal
Fil: Ségransan, D.. Universidad de Ginebra; Suiza
Fil: Strøm, P. A.. University of Warwick; Reino Unido
Fil: Udry, S.. Universidad de Ginebra; Suiza - Materia
-
ASTROMETRY
BROWN DWARFS
INSTRUMENTATION: SPECTROGRAPHS
PLANETARY SYSTEMS
STARS: LOW-MASS
TECHNIQUES: RADIAL VELOCITIES - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by/2.5/ar/
- Repositorio
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/154528
Ver los metadatos del registro completo
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The SOPHIE search for northern extrasolar planets: XVII. A wealth of new objects: Six cool Jupiters, three brown dwarfs, and 16 low-mass binary starsDalal, S.Kiefer, F.Hébrard, G.Sahlmann, J.Sousa, S.G.Forveille, T.Delfosse, X.Arnold, L.Astudillo Defru, NicolaBonfils, X.Boisse, I.Bouchy, F.Bourrier, V.Brugger, B.Cortés Zuleta, P.Deleuil, M.Demangeon, O. D. S.Díaz, Rodrigo FernandoHara, N. C.Heidari, N.Hobson, M. J.Lopez, T.Lovis, C.Martioli, E.Mignon, L.Mousis, O.Moutou, C.Rey, J.Santerne, A.Santos, N. C.Ségransan, D.Strøm, P. A.Udry, S.ASTROMETRYBROWN DWARFSINSTRUMENTATION: SPECTROGRAPHSPLANETARY SYSTEMSSTARS: LOW-MASSTECHNIQUES: RADIAL VELOCITIEShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Distinguishing classes within substellar objects and understanding their formation and evolution need larger samples of substellar companions such as exoplanets, brown dwarfs, and low-mass stars. In this paper, we look for substellar companions using radial velocity surveys of FGK stars with the SOPHIE spectrograph at the Observatoire de Haute-Provence. We assign here the radial velocity variations of 27 stars to their orbital motion induced by low-mass companions. We also constrained their plane-of-the-sky motion using HIPPARCOS and Gaia Data Release 1 measurements, which constrain the true masses of some of these companions. We report the detection and characterization of six cool Jupiters, three brown dwarf candidates, and 16 low-mass stellar companions. We additionally update the orbital parameters of the low-mass star HD 8291 B, and we conclude that the radial velocity variations of HD 204277 are likely due to stellar activity despite resembling the signal of a giant planet. One of the new giant planets, BD+631405 b, adds to the population of highly eccentric cool Jupiters, and it is presently the most massive member. Two of the cool Jupiter systems also exhibit signatures of an additional outer companion. The orbital periods of the new companions span 30 days to 11.5 yr, their masses 0.72 MJ-0.61 Ma, and their eccentricities 0.04-0.88. These discoveries probe the diversity of substellar objects and low-mass stars, which will help constrain the models of their formation and evolution.Fil: Dalal, S.. Institut d’Astrophysique de Paris; FranciaFil: Kiefer, F.. Institut d’Astrophysique de Paris; Francia. Centre National de la Recherche Scientifique. Observatoire de Paris; FranciaFil: Hébrard, G.. Université d’Aix-Marseille; Francia. Institut d’Astrophysique de Paris; FranciaFil: Sahlmann, J.. European Space Astronomy Centre; EspañaFil: Sousa, S.G.. Universidad de Porto; PortugalFil: Forveille, T.. Universite Grenoble Alpes; FranciaFil: Delfosse, X.. Universite Grenoble Alpes; FranciaFil: Arnold, L.. Université d’Aix-Marseille; FranciaFil: Astudillo Defru, Nicola. Universidad Católica de la Santísima Concepción; ChileFil: Bonfils, X.. Universite Grenoble Alpes; FranciaFil: Boisse, I.. Université d’Aix-Marseille; FranciaFil: Bouchy, F.. Universidad de Ginebra; SuizaFil: Bourrier, V.. Universidad de Ginebra; SuizaFil: Brugger, B.. Université d’Aix-Marseille; FranciaFil: Cortés Zuleta, P.. Université d’Aix-Marseille; FranciaFil: Deleuil, M.. Université d’Aix-Marseille; FranciaFil: Demangeon, O. D. S.. Universidad de Porto; PortugalFil: Díaz, Rodrigo Fernando. Consejo Nacional de Investigaciones Científicas y Técnicas. Instituto de Ciencias Físicas. - Universidad Nacional de San Martín. Instituto de Ciencias Físicas; Argentina. Universidad Nacional de San Martín. Escuela de Política y Gobierno; ArgentinaFil: Hara, N. C.. Universidad de Ginebra; SuizaFil: Heidari, N.. Universite de Nice-Sophia Antipolis. Laboratoire Joseph-louis Lagrange; Francia. Shahid Beheshti University; Irán. Université d’Aix-Marseille; FranciaFil: Hobson, M. J.. Pontificia Universidad Católica de Chile; Chile. Instituto Milenio de Astrofísica; ChileFil: Lopez, T.. Université d’Aix-Marseille; FranciaFil: Lovis, C.. Universidad de Ginebra; SuizaFil: Martioli, E.. Institut d’Astrophysique de Paris; Francia. Laboratório Nacional de Astrofísica; BrasilFil: Mignon, L.. Universidad Católica de la Santísima Concepción; ChileFil: Mousis, O.. Université d’Aix-Marseille; FranciaFil: Moutou, C.. Universite de Toulose - Le Mirail; FranciaFil: Rey, J.. Carnegie Institution of Washington. Las Campanas Observatory; ChileFil: Santerne, A.. Université d’Aix-Marseille; FranciaFil: Santos, N. C.. Universidad de Porto; PortugalFil: Ségransan, D.. Universidad de Ginebra; SuizaFil: Strøm, P. A.. University of Warwick; Reino UnidoFil: Udry, S.. Universidad de Ginebra; SuizaEDP Sciences2021-07-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/154528Dalal, S.; Kiefer, F.; Hébrard, G.; Sahlmann, J.; Sousa, S.G.; et al.; The SOPHIE search for northern extrasolar planets: XVII. A wealth of new objects: Six cool Jupiters, three brown dwarfs, and 16 low-mass binary stars; EDP Sciences; Astronomy and Astrophysics; 651; A11; 1-7-2021; 1-270004-63611432-0746CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/202140712info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/full_html/2021/07/aa40712-21/aa40712-21.htmlinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-10T13:23:44Zoai:ri.conicet.gov.ar:11336/154528instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-10 13:23:44.817CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
The SOPHIE search for northern extrasolar planets: XVII. A wealth of new objects: Six cool Jupiters, three brown dwarfs, and 16 low-mass binary stars |
| title |
The SOPHIE search for northern extrasolar planets: XVII. A wealth of new objects: Six cool Jupiters, three brown dwarfs, and 16 low-mass binary stars |
| spellingShingle |
The SOPHIE search for northern extrasolar planets: XVII. A wealth of new objects: Six cool Jupiters, three brown dwarfs, and 16 low-mass binary stars Dalal, S. ASTROMETRY BROWN DWARFS INSTRUMENTATION: SPECTROGRAPHS PLANETARY SYSTEMS STARS: LOW-MASS TECHNIQUES: RADIAL VELOCITIES |
| title_short |
The SOPHIE search for northern extrasolar planets: XVII. A wealth of new objects: Six cool Jupiters, three brown dwarfs, and 16 low-mass binary stars |
| title_full |
The SOPHIE search for northern extrasolar planets: XVII. A wealth of new objects: Six cool Jupiters, three brown dwarfs, and 16 low-mass binary stars |
| title_fullStr |
The SOPHIE search for northern extrasolar planets: XVII. A wealth of new objects: Six cool Jupiters, three brown dwarfs, and 16 low-mass binary stars |
| title_full_unstemmed |
The SOPHIE search for northern extrasolar planets: XVII. A wealth of new objects: Six cool Jupiters, three brown dwarfs, and 16 low-mass binary stars |
| title_sort |
The SOPHIE search for northern extrasolar planets: XVII. A wealth of new objects: Six cool Jupiters, three brown dwarfs, and 16 low-mass binary stars |
| dc.creator.none.fl_str_mv |
Dalal, S. Kiefer, F. Hébrard, G. Sahlmann, J. Sousa, S.G. Forveille, T. Delfosse, X. Arnold, L. Astudillo Defru, Nicola Bonfils, X. Boisse, I. Bouchy, F. Bourrier, V. Brugger, B. Cortés Zuleta, P. Deleuil, M. Demangeon, O. D. S. Díaz, Rodrigo Fernando Hara, N. C. Heidari, N. Hobson, M. J. Lopez, T. Lovis, C. Martioli, E. Mignon, L. Mousis, O. Moutou, C. Rey, J. Santerne, A. Santos, N. C. Ségransan, D. Strøm, P. A. Udry, S. |
| author |
Dalal, S. |
| author_facet |
Dalal, S. Kiefer, F. Hébrard, G. Sahlmann, J. Sousa, S.G. Forveille, T. Delfosse, X. Arnold, L. Astudillo Defru, Nicola Bonfils, X. Boisse, I. Bouchy, F. Bourrier, V. Brugger, B. Cortés Zuleta, P. Deleuil, M. Demangeon, O. D. S. Díaz, Rodrigo Fernando Hara, N. C. Heidari, N. Hobson, M. J. Lopez, T. Lovis, C. Martioli, E. Mignon, L. Mousis, O. Moutou, C. Rey, J. Santerne, A. Santos, N. C. Ségransan, D. Strøm, P. A. Udry, S. |
| author_role |
author |
| author2 |
Kiefer, F. Hébrard, G. Sahlmann, J. Sousa, S.G. Forveille, T. Delfosse, X. Arnold, L. Astudillo Defru, Nicola Bonfils, X. Boisse, I. Bouchy, F. Bourrier, V. Brugger, B. Cortés Zuleta, P. Deleuil, M. Demangeon, O. D. S. Díaz, Rodrigo Fernando Hara, N. C. Heidari, N. Hobson, M. J. Lopez, T. Lovis, C. Martioli, E. Mignon, L. Mousis, O. Moutou, C. Rey, J. Santerne, A. Santos, N. C. Ségransan, D. Strøm, P. A. Udry, S. |
| author2_role |
author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author |
| dc.subject.none.fl_str_mv |
ASTROMETRY BROWN DWARFS INSTRUMENTATION: SPECTROGRAPHS PLANETARY SYSTEMS STARS: LOW-MASS TECHNIQUES: RADIAL VELOCITIES |
| topic |
ASTROMETRY BROWN DWARFS INSTRUMENTATION: SPECTROGRAPHS PLANETARY SYSTEMS STARS: LOW-MASS TECHNIQUES: RADIAL VELOCITIES |
| purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| dc.description.none.fl_txt_mv |
Distinguishing classes within substellar objects and understanding their formation and evolution need larger samples of substellar companions such as exoplanets, brown dwarfs, and low-mass stars. In this paper, we look for substellar companions using radial velocity surveys of FGK stars with the SOPHIE spectrograph at the Observatoire de Haute-Provence. We assign here the radial velocity variations of 27 stars to their orbital motion induced by low-mass companions. We also constrained their plane-of-the-sky motion using HIPPARCOS and Gaia Data Release 1 measurements, which constrain the true masses of some of these companions. We report the detection and characterization of six cool Jupiters, three brown dwarf candidates, and 16 low-mass stellar companions. We additionally update the orbital parameters of the low-mass star HD 8291 B, and we conclude that the radial velocity variations of HD 204277 are likely due to stellar activity despite resembling the signal of a giant planet. One of the new giant planets, BD+631405 b, adds to the population of highly eccentric cool Jupiters, and it is presently the most massive member. Two of the cool Jupiter systems also exhibit signatures of an additional outer companion. The orbital periods of the new companions span 30 days to 11.5 yr, their masses 0.72 MJ-0.61 Ma, and their eccentricities 0.04-0.88. These discoveries probe the diversity of substellar objects and low-mass stars, which will help constrain the models of their formation and evolution. Fil: Dalal, S.. Institut d’Astrophysique de Paris; Francia Fil: Kiefer, F.. Institut d’Astrophysique de Paris; Francia. Centre National de la Recherche Scientifique. Observatoire de Paris; Francia Fil: Hébrard, G.. Université d’Aix-Marseille; Francia. Institut d’Astrophysique de Paris; Francia Fil: Sahlmann, J.. European Space Astronomy Centre; España Fil: Sousa, S.G.. Universidad de Porto; Portugal Fil: Forveille, T.. Universite Grenoble Alpes; Francia Fil: Delfosse, X.. Universite Grenoble Alpes; Francia Fil: Arnold, L.. Université d’Aix-Marseille; Francia Fil: Astudillo Defru, Nicola. Universidad Católica de la Santísima Concepción; Chile Fil: Bonfils, X.. Universite Grenoble Alpes; Francia Fil: Boisse, I.. Université d’Aix-Marseille; Francia Fil: Bouchy, F.. Universidad de Ginebra; Suiza Fil: Bourrier, V.. Universidad de Ginebra; Suiza Fil: Brugger, B.. Université d’Aix-Marseille; Francia Fil: Cortés Zuleta, P.. Université d’Aix-Marseille; Francia Fil: Deleuil, M.. Université d’Aix-Marseille; Francia Fil: Demangeon, O. D. S.. Universidad de Porto; Portugal Fil: Díaz, Rodrigo Fernando. Consejo Nacional de Investigaciones Científicas y Técnicas. Instituto de Ciencias Físicas. - Universidad Nacional de San Martín. Instituto de Ciencias Físicas; Argentina. Universidad Nacional de San Martín. Escuela de Política y Gobierno; Argentina Fil: Hara, N. C.. Universidad de Ginebra; Suiza Fil: Heidari, N.. Universite de Nice-Sophia Antipolis. Laboratoire Joseph-louis Lagrange; Francia. Shahid Beheshti University; Irán. Université d’Aix-Marseille; Francia Fil: Hobson, M. J.. Pontificia Universidad Católica de Chile; Chile. Instituto Milenio de Astrofísica; Chile Fil: Lopez, T.. Université d’Aix-Marseille; Francia Fil: Lovis, C.. Universidad de Ginebra; Suiza Fil: Martioli, E.. Institut d’Astrophysique de Paris; Francia. Laboratório Nacional de Astrofísica; Brasil Fil: Mignon, L.. Universidad Católica de la Santísima Concepción; Chile Fil: Mousis, O.. Université d’Aix-Marseille; Francia Fil: Moutou, C.. Universite de Toulose - Le Mirail; Francia Fil: Rey, J.. Carnegie Institution of Washington. Las Campanas Observatory; Chile Fil: Santerne, A.. Université d’Aix-Marseille; Francia Fil: Santos, N. C.. Universidad de Porto; Portugal Fil: Ségransan, D.. Universidad de Ginebra; Suiza Fil: Strøm, P. A.. University of Warwick; Reino Unido Fil: Udry, S.. Universidad de Ginebra; Suiza |
| description |
Distinguishing classes within substellar objects and understanding their formation and evolution need larger samples of substellar companions such as exoplanets, brown dwarfs, and low-mass stars. In this paper, we look for substellar companions using radial velocity surveys of FGK stars with the SOPHIE spectrograph at the Observatoire de Haute-Provence. We assign here the radial velocity variations of 27 stars to their orbital motion induced by low-mass companions. We also constrained their plane-of-the-sky motion using HIPPARCOS and Gaia Data Release 1 measurements, which constrain the true masses of some of these companions. We report the detection and characterization of six cool Jupiters, three brown dwarf candidates, and 16 low-mass stellar companions. We additionally update the orbital parameters of the low-mass star HD 8291 B, and we conclude that the radial velocity variations of HD 204277 are likely due to stellar activity despite resembling the signal of a giant planet. One of the new giant planets, BD+631405 b, adds to the population of highly eccentric cool Jupiters, and it is presently the most massive member. Two of the cool Jupiter systems also exhibit signatures of an additional outer companion. The orbital periods of the new companions span 30 days to 11.5 yr, their masses 0.72 MJ-0.61 Ma, and their eccentricities 0.04-0.88. These discoveries probe the diversity of substellar objects and low-mass stars, which will help constrain the models of their formation and evolution. |
| publishDate |
2021 |
| dc.date.none.fl_str_mv |
2021-07-01 |
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info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
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article |
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publishedVersion |
| dc.identifier.none.fl_str_mv |
http://hdl.handle.net/11336/154528 Dalal, S.; Kiefer, F.; Hébrard, G.; Sahlmann, J.; Sousa, S.G.; et al.; The SOPHIE search for northern extrasolar planets: XVII. A wealth of new objects: Six cool Jupiters, three brown dwarfs, and 16 low-mass binary stars; EDP Sciences; Astronomy and Astrophysics; 651; A11; 1-7-2021; 1-27 0004-6361 1432-0746 CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/154528 |
| identifier_str_mv |
Dalal, S.; Kiefer, F.; Hébrard, G.; Sahlmann, J.; Sousa, S.G.; et al.; The SOPHIE search for northern extrasolar planets: XVII. A wealth of new objects: Six cool Jupiters, three brown dwarfs, and 16 low-mass binary stars; EDP Sciences; Astronomy and Astrophysics; 651; A11; 1-7-2021; 1-27 0004-6361 1432-0746 CONICET Digital CONICET |
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eng |
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eng |
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info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/202140712 info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/full_html/2021/07/aa40712-21/aa40712-21.html |
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info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by/2.5/ar/ |
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openAccess |
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https://creativecommons.org/licenses/by/2.5/ar/ |
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application/pdf application/pdf |
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EDP Sciences |
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EDP Sciences |
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CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
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dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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