Occurrence and Architecture of Kepler Planetary Systems as Functions of Stellar Mass and Effective Temperature
The Kepler mission has discovered thousands of exoplanets around various stars with different spectral types (M, K, G, and F) and thus different masses and effective temperatures. Previous studies have shown that the planet occurrence rate, in terms of the average number of planets per star, drops w...
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Veröffentlicht in: | The Astronomical journal 2020-04, Vol.159 (4), p.164 |
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