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Characterization of exoplanets from their formation III: The statistics of planetary luminosities
C. Mordasini, G. -D. Marleau, P. Mollière
This paper continues a series in which we predict the main observable characteristics of exoplanets based on their formation. In Paper I we described our global planet formation an…
High signal-to-noise spectral characterization of the planetary-mass object HD 106906 b
Sebastian Daemgen, Kamen Todorov, Sascha P. Quanz +4
We spectroscopically characterize the atmosphere of HD 106906b, a young low-mass companion near the deuterium burning limit. The wide separation from its host star of 7.1" makes it…
Discovery of a warm, dusty giant planet around HIP65426
G. Chauvin, S. Desidera, A. -M. Lagrange +120
The SHINE program is a large high-contrast near-infrared survey of 600 young, nearby stars. It is aimed at searching for and characterizing new planetary systems using VLT/SPHERE's…
The Planetary Accretion Shock: I. Framework for Radiation-hydrodynamical Simulations and First Results
Gabriel-Dominique Marleau, Hubert Klahr, Rolf Kuiper +1
The key aspect determining the post-formation luminosity of gas giants has long been considered to be the energetics of the accretion shock at the planetary surface. We use 1D radi…