Revising the properties of low mass eclipsing binary stars using TESS light curves
Maxted, P. F. L.; Southworth, J.; Mancini, L.; Jennings, Z.
United Kingdom, Italy, Germany
Abstract
Precise measurements of stellar parameters are required in order to develop our theoretical understanding of stellar structure. These measurements enable errors and uncertainties to be quantified in theoretical models and constrain the physical interpretation of observed phenomena, such as the inflated radii of low-mass stars.