eccentric planets

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Today, formation theory cannot explain all these observed characteristics in one coherent picture. But at least for some observations, theory can give us ideas about possible mechanisms responsible for them.
6.1 a-M diagram
Page 1 and 2: Observational constraints from the
Page 3 and 4: 6. Properties of extrasolar planets
Page 5 and 6: Different techniques - different co
Page 7: Overview on observed exoplanet prop
Page 11 and 12: Frequency of planet types Bias-corr
Page 13 and 14: ∼15 MJup, with an upper mass limi
Page 15 and 16: Grether & Lineweaver 2006 Mass dist
Page 17 and 18: ative points of view invoke in situ
Page 19 and 20: 6.4 Eccentricity distribution
Page 21 and 22: 6.5 Metallicity
Page 23 and 24: N. Santos et al. (2005) Metallicity
Page 25 and 26: Sousa et al. 2011 Metallicity effec
Page 27 and 28: Influence of the host star mass •
Page 29 and 30: Multiplicity •Fraction of giant p
Page 31 and 32: Kepler multiple systems •Kepler h
Page 33 and 34: or stems directly from 35% rms unce
Page 35 and 36: M-R: Giant planets •During evolut
Page 37 and 38: Additional observations
Page 39 and 40: Transits: correlation planetary cor

eccentric planets

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