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

Autor: Patrick Guillout, Tsevi Mazeh, Yveline Lebreton, Jean-Baptiste Le Bouquin, Benoit Famaey, F. Kiefer, Frédéric Arenou, J.-B. Salomon, Henri M. J. Boffin, Jean-Louis Halbwachs, Dimitri Pourbaix

Publikováno v: Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2020, 496 (2), pp.1355-1368. ⟨10.1093/mnras/staa1571⟩
Monthly notices of the Royal Astronomical Society, 496 (2
Monthly Notices of the Royal Astronomical Society, 2020, 496 (2), pp.1355-1368. ⟨10.1093/mnras/staa1571⟩

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 r

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https://hal.archives-ouvertes.fr/hal-02881420/document