Gone with the headwind : planetesimals on eccentric orbits erode rapidly
CEDENBLAD L., SCHFFER N., JOHANSEN A., MEHLIG B. & MITRA D.
ApJ
, submitted
arxiv
Spatial distribution of the aromatic and aliphatic carbonaceous nano-grain features in the protoplanetary disk around HD 100546
HABART E., BOUTERAON Th., BRAUER R., YSARD N., PANTIN E. et al.
Astron. & Astrophys.
, accepted
arxiv
Observational constraints on the likelihood of 26Al in planet-forming environments
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MIRACLES: atmospheric characterization of directly imaged planets and substellar companions at 4-5 μm. II. Constraints on the mass and radius of the enshrouded planet PDS 70 b
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A close-encounter method for simulating the dynamics of planetesimals
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Variable refractory lithophile element compositions of planetary building blocks
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arxiv
Stability analysis of three exoplanet systems
MARSHALL J., HORNER J., WITTENMYER R., CLARK J. & MENGEL M.
MNRAS
, accepted
arxiv
A Search for Polarized Thermal Emission from Directly Imaged Exoplanets and Brown Dwarf Companions to Nearby Stars
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Losing Oceans: The Effects of Composition on the Thermal Component of Impact-driven Atmospheric Loss
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Can Large-Scale Migration Explain the Giant Planet Occurrence Rate?
Beyond Equilibrium Temperature: How the Atmosphere/Interior Connection Affects the Onset of Methane, Ammonia, and Clouds in Warm Transiting Giant Planets
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A Closer Look at Exoplanet Occurrence Rates: Considering the Multiplicity of Stars Without Detected Planets
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OWL-Moon in 2050 and Beyond
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Probing the impact of varied migration and gas accretion rates for the formation of giant planets in the pebble accretion scenario
NDUGU N., BITSCH B., MORBIDELLI A., CRIDA A. & JURUA E.
MNRAS
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paperarxiv
Hiding Signatures of Gravitational Instability in Protoplanetary Discs with Planets
ROWTHER S., MERU F., KENNEDY G., NEALON R. & PINTE Ch.
ApJ Lett.
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paperarxiv
Architectures of Exoplanetary Systems: Eccentricity and Mutual Inclination Distributions of AMD-Stable Planetary Systems
HE M., FORD E., RAGOZZINE D. & CARRERA D.
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An Unusual Transmission Spectrum for the Sub-Saturn KELT-11b Suggestive of a Sub-Solar Water Abundance
COLON K., KREIDBERG L., LINE M., WELBANKS L., MADHUSUDHAN N., et al.
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XAO-assisted coronagraphy with SHARK NIR: from simulations to laboratory tests
UMBRIACO G., CAROLO E., VASSALLO D., FARINATO J., BAUDOZ P. et al.
arxiv
Revisiting migration in a disc cavity to explain the high eccentricities of warm Jupiters