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...
| Prif Awdur: | |
|---|---|
| Awduron Eraill: | |
| Fformat: | Traethawd Ymchwil |
| Iaith: | English |
| Cyhoeddwyd: |
2021
|
| Pynciau: |