The SOPHIE search for northern extrasolar planets: XII. Three giant planets suitable for astrometric mass determination with Gaia

We present new radial velocity measurements for three low-metallicity solar-like stars observed with the SOPHIE spectrograph and its predecessor ELODIE, both installed at the 193 cm telescope of the Haute-Provence Observatory, allowing the detection and characterization of three new giant extrasolar...

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Autor principal:	Díaz, Rodrigo Fernando
Publicado:	2017
Materias:	brown dwarfs planetary systems stars: individual: HD17674 stars: individual: HD29021 stars: individual: HD42012 techniques: radial velocities Planets Satellites Stars Brown dwarfs Intermediate periods Mass determination Planetary system Radial velocity measurements Solar-like stars Stars: individual Techniques: radial velocities Extrasolar planets
Acceso en línea:	https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v601_n_p_Rey http://hdl.handle.net/20.500.12110/paper_00046361_v601_n_p_Rey
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

id	paper:paper_00046361_v601_n_p_Rey
record_format	dspace
spelling	paper:paper_00046361_v601_n_p_Rey2023-06-08T14:28:19Z The SOPHIE search for northern extrasolar planets: XII. Three giant planets suitable for astrometric mass determination with Gaia Díaz, Rodrigo Fernando brown dwarfs planetary systems stars: individual: HD17674 stars: individual: HD29021 stars: individual: HD42012 techniques: radial velocities Planets Satellites Stars Brown dwarfs Intermediate periods Mass determination Planetary system Radial velocity measurements Solar-like stars Stars: individual Techniques: radial velocities Extrasolar planets We present new radial velocity measurements for three low-metallicity solar-like stars observed with the SOPHIE spectrograph and its predecessor ELODIE, both installed at the 193 cm telescope of the Haute-Provence Observatory, allowing the detection and characterization of three new giant extrasolar planets in intermediate periods of 1.7 to 3.7 yr. All three stars, HD 17674, HD 42012 and HD 29021 present single giant planetary companions with minimum masses between 0.9 and 2.5 M Jup . The range of periods and masses of these companions, along with the distance of their host stars, make them good targets to look for astrometric signals over the lifetime of the new astrometry satellite Gaia. We discuss the preliminary astrometric solutions obtained from the first Gaia data release. © ESO, 2017. Fil:Díaz, R.F. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. 2017 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v601_n_p_Rey http://hdl.handle.net/20.500.12110/paper_00046361_v601_n_p_Rey
institution	Universidad de Buenos Aires
institution_str	I-28
repository_str	R-134
collection	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic	brown dwarfs planetary systems stars: individual: HD17674 stars: individual: HD29021 stars: individual: HD42012 techniques: radial velocities Planets Satellites Stars Brown dwarfs Intermediate periods Mass determination Planetary system Radial velocity measurements Solar-like stars Stars: individual Techniques: radial velocities Extrasolar planets
spellingShingle	brown dwarfs planetary systems stars: individual: HD17674 stars: individual: HD29021 stars: individual: HD42012 techniques: radial velocities Planets Satellites Stars Brown dwarfs Intermediate periods Mass determination Planetary system Radial velocity measurements Solar-like stars Stars: individual Techniques: radial velocities Extrasolar planets Díaz, Rodrigo Fernando The SOPHIE search for northern extrasolar planets: XII. Three giant planets suitable for astrometric mass determination with Gaia
topic_facet	brown dwarfs planetary systems stars: individual: HD17674 stars: individual: HD29021 stars: individual: HD42012 techniques: radial velocities Planets Satellites Stars Brown dwarfs Intermediate periods Mass determination Planetary system Radial velocity measurements Solar-like stars Stars: individual Techniques: radial velocities Extrasolar planets
description	We present new radial velocity measurements for three low-metallicity solar-like stars observed with the SOPHIE spectrograph and its predecessor ELODIE, both installed at the 193 cm telescope of the Haute-Provence Observatory, allowing the detection and characterization of three new giant extrasolar planets in intermediate periods of 1.7 to 3.7 yr. All three stars, HD 17674, HD 42012 and HD 29021 present single giant planetary companions with minimum masses between 0.9 and 2.5 M Jup . The range of periods and masses of these companions, along with the distance of their host stars, make them good targets to look for astrometric signals over the lifetime of the new astrometry satellite Gaia. We discuss the preliminary astrometric solutions obtained from the first Gaia data release. © ESO, 2017.
author	Díaz, Rodrigo Fernando
author_facet	Díaz, Rodrigo Fernando
author_sort	Díaz, Rodrigo Fernando
title	The SOPHIE search for northern extrasolar planets: XII. Three giant planets suitable for astrometric mass determination with Gaia
title_short	The SOPHIE search for northern extrasolar planets: XII. Three giant planets suitable for astrometric mass determination with Gaia
title_full	The SOPHIE search for northern extrasolar planets: XII. Three giant planets suitable for astrometric mass determination with Gaia
title_fullStr	The SOPHIE search for northern extrasolar planets: XII. Three giant planets suitable for astrometric mass determination with Gaia
title_full_unstemmed	The SOPHIE search for northern extrasolar planets: XII. Three giant planets suitable for astrometric mass determination with Gaia
title_sort	sophie search for northern extrasolar planets: xii. three giant planets suitable for astrometric mass determination with gaia
publishDate	2017
url	https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v601_n_p_Rey http://hdl.handle.net/20.500.12110/paper_00046361_v601_n_p_Rey
work_keys_str_mv	AT diazrodrigofernando thesophiesearchfornorthernextrasolarplanetsxiithreegiantplanetssuitableforastrometricmassdeterminationwithgaia AT diazrodrigofernando sophiesearchfornorthernextrasolarplanetsxiithreegiantplanetssuitableforastrometricmassdeterminationwithgaia
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The SOPHIE search for northern extrasolar planets: XII. Three giant planets suitable for astrometric mass determination with Gaia

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