2 papers
astro-ph.EP2024
A new mass and radius determination of the ultra-short period planet K2-106b and the fluffy planet K2-106c
E. W. Guenther, E. Goffo, D. Sebastian +5
Ultra-short period planets have orbital periods of less than one day. Since their masses and radii can be determined to a higher precision than long-period planets, they are the pr…
astro-ph.SR2023
The EBLM Project XI. Mass, radius and effective temperature measurements for 23 M-dwarf companions to solar-type stars observed with CHEOPS
M. I. Swayne, P. F. L. Maxted, A. H. M. J. Triaud +104
Observations of low-mass stars have frequently shown a disagreement between observed stellar radii and radii predicted by theoretical stellar structure models. This ``radius inflat…