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...
第一著者: | Zicher, N |
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その他の著者: | Aigrain, S |
フォーマット: | 学位論文 |
言語: | English |
出版事項: |
2021
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主題: |
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