Identifying the "true" radius of the hot sub-Neptune CoRoT-24b by mass loss modelling

H. Lammer, N. V. Erkaev, L. Fossati +8

For the hot exoplanets CoRoT-24b and CoRoT-24c, observations have provided transit radii R${}_{\mathrm{T}}$ of 3.7$\pm$0.4 R${}_{\oplus }$ and 4.9$\pm$0.5 R${}_{\oplus }$, and masses of $\le$5.…