http://arxiv.org/abs/1912.13400
I present a brief summary of three different types of binary star – astrometric, spectroscopic and eclipsing – and tabulate the properties of these systems that can be determined directly from observations. Eclipsing binary stars are the most valuable of these, as they are our main source of direct mass and radius measurements for normal stars. In good cases, masses and radii can be obtained to better than 1% precision and accuracy using only photometry, spectroscopy and geometry. These measurements constitute vital empirical data against which theoretical models of stars can be verified and improved. I give examples of the use of these systems for constraining stellar theory and the distance scale, and conclude with a presentation of preliminary results for the solar-type eclipsing binary 1SWASP J034114.25+201253.5.
J. Southworth
Wed, 1 Jan 20
26/88
Comments: 6 pages, 1 figure. Invited review for the BRITE Vienna conference, August 2019