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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| स्वरूप: | थीसिस |
| भाषा: | English |
| प्रकाशित: |
2021
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| विषय: |