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...

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Autore principale: Zicher, N
Altri autori: Aigrain, S
Natura: Tesi
Lingua:English
Pubblicazione: 2021
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