The EBLM Project VI. The mass and radius of five low-mass stars in F+M binaries discovered by the WASP survey
The EBLM Project VI. The mass and radius of five low-mass stars in F+M binaries discovered by the WASP survey
Some M-dwarfs around F-/G-type stars have been measured to be hotter and larger than predicted by stellar evolution models. Inconsistencies between observations and models need to be addressed with more mass, radius, and luminosity measurements of low-mass stars to test and refine evolutionary models. Our aim is to measure the …