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...
主要作者: | Zicher, N |
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其他作者: | Aigrain, S |
格式: | Thesis |
语言: | English |
出版: |
2021
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主题: |
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