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...

Полное описание

Библиографические подробности
Главный автор:	Zicher, N
Другие авторы:	Aigrain, S
Формат:	Диссертация
Язык:	English
Опубликовано:	2021
Предметы:	Extrasolar planets Stellar activity Extrasolar planets > Detection Gaussian processes Stars > Motion in line of sight Astrophysics

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