6533b874fe1ef96bd12d61ad
RESEARCH PRODUCT
The AB Doradus system revisited: The dynamical mass of AB Dor A/C
Ivan Marti-vidalJohn ReynoldsEduardo RosEduardo RosJ. C. GuiradoJ.-f. LestradeJ. M. MarcaideDavid L. JaunceyDavid L. JaunceyRebecca AzulayRebecca AzulayEmanuele Tognellisubject
Physics[PHYS]Physics [physics]010308 nuclear & particles physicsCalibration (statistics)Component (thermodynamics)AstronomyAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrometryAstrophysics01 natural sciencesStarsInterferometry13. Climate actionSpace and Planetary Science0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsComputingMilieux_MISCELLANEOUSdescription
We report new radio interferometric observations of the quadruple pre-main-sequence (PMS) system ABD oradus. From these observations, combined with existing VLT near-infrared relative astrometry, we have refined the estimates of the dynamical masses of the system. In particular, we find component masses of 0.86 ± 0.09M⊙ and 0.090 ± 0.003M⊙ for ABD or A and ABD or C, respectively. These dynamical masses, coupled with temperatures and luminosities, allow for comparison with theoretical stellar models. The case of ABDorC, in terms of calibration of evolutionary models of low-mass young stars has been widely reported in previous studies. In this contribution, we compare the measured properties of ABDorA with several solar-composition models for PMS stars. The models used in this comparison predict the dynamical mass to within the quoted uncertainties.
| year | journal | country | edition | language |
|---|---|---|---|---|
| 2017-11-01 |