A. Cumming
| The primordial entropy of Jupiter |
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A. Khan
| A generalized Bayesian inference method for constraining the interiors of super Earths and sub-Neptunes |
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A. Rivoldini
| A generalized Bayesian inference method for constraining the interiors of super Earths and sub-Neptunes |
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C. Dorn
C. Mordasini
Caroline Dorn
| Why do more massive stars host larger planets? |
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F. Masset
| The importance of thermal torques on the migration of planets growing by pebble accretion |
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F. Roig
| Origin and sustainability of the population of asteroids captured in the exterior resonance 1:2 with Mars |
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Illaria Pascucci
| Why do more massive stars host larger planets? |
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J. Cuadra
| The importance of thermal torques on the migration of planets growing by pebble accretion |
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J. Haldemann
| The nature of the radius valley. Hints from formation and evolution models. |
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J. Venturini
Julia Venturini
| Why do more massive stars host larger planets? |
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K. Heng
| A generalized Bayesian inference method for constraining the interiors of super Earths and sub-Neptunes |
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L. Mayer
| The formation of Jupiter by hybrid pebble-planetesimal accretion. |
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L. Senecal
| The formation of Jupiter by hybrid pebble-planetesimal accretion. |
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M. Ikoma
| Critical core mass for enriched envelopes: the role of $H_2O$ condensation |
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M. Lozovsky
| Threshold radii of volatile-rich planets |
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M. M. Miller Bertolami
| The importance of thermal torques on the migration of planets growing by pebble accretion |
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M. Miller-Bertolami.
| Giant planet formation at the pressure maxima of protoplanetary disks II. A hybrid accretion scenario |
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M. P. Ronco
M. Schönbächler
| The formation of Jupiter by hybrid pebble-planetesimal accretion. |
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Michael Lozovsky
| Why do more massive stars host larger planets? |
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N. Hikel
| Bayesian analysis of interiors of HD 219134b, Kepler-10b, Kepler-93b, CoRoT-7b, 55 Cnc e, and HD 97658b using stellar abundance proxies |
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O. M. Guilera
R. Burn
| The formation of Jupiter by hybrid pebble-planetesimal accretion. |
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R. Gil-Hutton
| Origin and sustainability of the population of asteroids captured in the exterior resonance 1:2 with Mars |
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R. Helled
Ravit Helled
| Why do more massive stars host larger planets? |
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Robert Feldmann
| Why do more massive stars host larger planets? |
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S. Ataiee
| Planet Formation, Migration and Habitability | |
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| The formation of Jupiter by hybrid pebble-planetesimal accretion. |
S. P. Quanz
| The formation of Jupiter by hybrid pebble-planetesimal accretion. |
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T. Gallardo
| Origin and sustainability of the population of asteroids captured in the exterior resonance 1:2 with Mars | |
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| How to take into account the relativistic effects in dynamical studies of comets |
W. Benz
Y. Alibert
Z. Sándor
| Giant planet formation at the pressure maxima of protoplanetary disks II. A hybrid accretion scenario |
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