Measuring the masses of planets around young active stars

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...

Bibliografski detalji
Glavni autor:	Zicher, N
Daljnji autori:	Aigrain, S
Format:	Disertacija
Jezik:	English
Izdano:	2021
Teme:	Extrasolar planets Stellar activity Extrasolar planets > Detection Gaussian processes Stars > Motion in line of sight Astrophysics

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