Measuring the masses of planets around young active stars
A quarter century after the famous discovery of 51 Peg b, the radial velocity (RV) method remains a key exoplanet detection and characterisation method. For transiting planets, RVs allow us to measure mean densities and draw conclusions about the planets’ compositions. This is particularly valuable...
| Autor principal: | |
|---|---|
| Otros Autores: | |
| Formato: | Tesis |
| Lenguaje: | English |
| Publicado: |
2021
|
| Materias: |