Accurate SB2 orbits for 10 binaries and masses of the components of 5 binaries (2020)
Available
Dataset
Licence : CC BY-NC-SA doi:10.25666/DATAOSU-2021-06-21 bibcode:2020yCat..74961355H vizier:J/MNRAS/496/1355
Data creators :
Jean-Louis Halbwachs [1],
Flavien Kiefer [2],
Yveline Lebreton [3],
Henri M. J. Boffin [4],
Frédéric Arenou [5],
Jean-Baptiste Le Bouquin [6],
Benoit Famaey [1],
Dimitri Pourbaix [7],
Patrick Guillout [1],
Jean-Baptiste Salomon [8] [9],
Tsevi Mazeh [10]
[1] : Observatoire astronomique de Strasbourg (UMR 7550)
[2] : Institut d'Astrophysique de Paris (UMR 7095)
[3] : Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique (UMR 8109)
[4] : European Southern Observatory
[5] : Galaxies, Etoiles, Physique, Instrumentation (UMR 8111)
[6] : Institut de Planétologie et d'Astrophysique de Grenoble (UMR 5274)
[7] : Institut d'Astronomie et d'Astrophyque - Université Libre de Bruxelles
[8] : Institut UTINAM (UMR 6213) (Université de Franche-Comté)
[9] : Observatoire des Sciences de l'Univers - Terre, Homme, Environnement, Temps, Astronomie (UAR 3245) (Université de Franche-Comté)
[10] : School of Physics and Astronomy - Tel Aviv University
Description :
Double-lined spectroscopic binaries (SB2s) are one of the main sources of stellar masses, as additional observations are only needed to give the inclinations of the orbital planes in order to obtain the individual masses of the components. For this reason, we are observing a selection of SB2s using the SOPHIE spectrograph at the Haute-Provence observatory in order to precisely determine their orbital elements. Our objective is to finally obtain masses with an accuracy of the order of one percent by combining our radial velocity (RV) measurements and the astrometric measurements that will come from the Gaia satellite. We present here the RVs and the re-determined orbits of 10 SB2s. In order to verify the masses we will derive from Gaia, we obtained interferometric measurements of the ESO VLTI for one of these SB2s. Adding the interferometric or speckle measurements already published by us or by others for 4 other stars, we finally obtain the masses of the components of 5 binary stars, with masses ranging from 0.51 to 2.2 solar masses, including main-sequence dwarfs and some more evolved stars whose location in the HR diagram has been estimated.
Discipline :
astronomy & astrophysics (sciences of the universe)
General metadata
Data acquisition date :
from 28 Oct 2006 to 21 Aug 2018
Data acquisition methods :
- Derived or compiled data : The RVs of the components are derived using the TwO-Dimensional CORrelation algorithm todcor (Zucker & Mazeh 1994ApJ...420..806Z; Zucker et al. 2004, Cat. J/A+A/426/695).
- Observational data : 10 spectroscopic binary stars (SB2s) were observed using the SOPHIE spectrograph at the Haute-Provence observatory (France) in order to precisely determine their orbital elements. These observations were complemented by interferometric measurements of the ESO VLTI for one of these SB2s and by interferometric or speckle measurements already published by us or by others for 4 other stars.
Formats :
application/fits, application/x-votable+xml, text/csv, text/html, text/plain, text/tab-separated-values, text/xml
Audience :
Research
Coverages
Spatial coverage :
- HIP 20601: right ascension 4h 24' 43", declination 4° 41' 59" N
- HIP 73449: right ascension 15h 0' 34", declination 8° 36' 0" N
- HIP 76006: right ascension 15h 31' 22", declination 36° 36' 59" N
- HIP 77725: right ascension 15h 52' 8", declination 10° 52' 28" N
- HIP 96656 : right ascension 19h 39' 6", declination 76° 25' 19" N
- HIP 104987: right ascension 21h 15' 49", declination 5° 14' 52" N
- HIP 117186: right ascension 23h 45' 37", declination 13° 9' 9" N
- HIP 7134: right ascension 1h 31' 54", declination 16° 2' 49" N
- HIP 61732: right ascension 12h 39' 12", declination 16° 30' 36" N
- HIP 101452: right ascension 20h 33' 39", declination 45° 10' 32" N
Publications :
- Masses of the components of SB2 binaries observed with Gaia – V. Accurate SB2 orbits for 10 binaries and masses of the components of 5 binaries (doi:10.1093/mnras/staa1571)
Publisher :
Centre des Données astronomiques de Strasbourg
Record created 21 Jun 2021 by Jean-Baptiste Salomon.
Local identifier: FR-18008901306731-2021-06-21.
