0000000001037175

AUTHOR

D. Jauncey

showing 1 related works from this author

Dynamical masses of the low-mass stellar binary AB Doradus B

2015

Context. ABDoradus is the main system of the ABDoradus moving group. It is a quadruple system formed by two widely separated binaries of pre-main-sequence (PMS) stars: ABDor A/C and ABDor Ba/Bb. The pair ABDor A/C has been extensively studied and its dynamical masses have been determined with high precision, thus making of ABDor C a benchmark for calibrating PMS stellar models. If the orbit and dynamical masses of the pair ABDor Ba/Bb can be determined, they could not only play a similar role to that of ABDor C in calibrating PMS models, but would also help to better understand the dynamics of the whole ABDoradus system. Aims. We aim to determine the individual masses of the pair ABDor Ba/B…

Orbital elementsPhysicsAstrofísica[PHYS]Physics [physics]InfraredFOS: Physical sciencesBinary numberAstronomy and AstrophysicsContext (language use)AstrophysicsStarsAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceVery-long-baseline interferometryOrbit (dynamics)AstronomiaLow Mass[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Solar and Stellar Astrophysics (astro-ph.SR)ComputingMilieux_MISCELLANEOUS
researchProduct