Skip navigation
Skip navigation

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

Azulay, R; Guirado, J.C.; Marcaide, J.M.; Mart-Vidal, I; Ros, E; Jauncey, David; Lestrade, J.F.; Preston, R.A.; Reynolds, J E; Tognelli, E; Ventura, P

Description

Context. AB Doradus is the main system of the AB Doradus moving group. It is a quadruple system formed by two widely separated binaries of pre-main-sequence (PMS) stars: AB Dor A/C and AB Dor Ba/Bb. The pair AB Dor A/C has been extensively studied and its dynamical masses have been determined with high precision, thus making AB Dor C a benchmark for calibrating PMS stellar models. If the orbit and dynamical masses of the pair AB Dor Ba/Bb could be determined, they could play a similar role to...[Show more]

CollectionsANU Research Publications
Date published: 2015
Type: Journal article
URI: http://hdl.handle.net/1885/102623
Source: Astronomy and Astrophysics
DOI: 10.1051/0004-6361/201525704

Download

File Description SizeFormat Image
01_Azulay_Dynamical_masses_of_the_2015.pdf315.99 kBAdobe PDF    Request a copy


Items in Open Research are protected by copyright, with all rights reserved, unless otherwise indicated.

Updated:  20 July 2017/ Responsible Officer:  University Librarian/ Page Contact:  Library Systems & Web Coordinator