Results 11 to 20 of about 708 (150)
Orbital misalignment of the GJ 436b exoplanet. Constraints on the Kozai migration scenario
Kozai-Lidov mechanism is a major source of dynamical evolution in multiple stellar systems and in young planetary systems with large mutual inclinations.
Vincent Bourrier +7 more
core +2 more sources
Comparative studies of young and old exoplanet populations offer a glimpse into how planets may form and evolve with time. We present an occurrence rate study of short-period (
Rachel B. Fernandes +21 more
core +5 more sources
Orbital migration and the period distribution of exoplanets [PDF]
published in A& ...
DEL POPOLO A, ERCAN N, YE, ILYURT IS.
openaire +5 more sources
Statistical properties of exoplanets [PDF]
Accepted in A& ...
Udry, S., Mayor, M., Santos, N. C.
openaire +2 more sources
PROTOSTELLAR CLOUD FRAGMENTATION AND INWARD MIGRATION BY DISK CAPTURE AS THE ORIGIN OF MASSIVE EXOPLANETS [PDF]
A new model for the formation of Jovian planets is proposed. We consider planets forming at large distances from a protostar (>100 AU) through direct fragmentation of a gas cloud, by the same formation mechanism as wide stellar and brown dwarf binaries. We model the gravitational evolution of a system of these distant planets and a second population
Font-Ribera, A. +2 more
openaire +2 more sources
How many suns are in the sky? A SPHERE multiplicity survey of exoplanet host stars [PDF]
Aims. We are studying the influence of stellar multiplicity on exoplanet systems and, in particular, systems that have been detected via radial-velocity searches.
R. G. van Holstein +11 more
core +1 more source
Nuclear Processes in Dark Interstellar Matter of H(0) Decrease the Hope of Migrating to Exoplanets [PDF]
It is still generally assumed that interstellar travel will be possible after purely technical development and thus that mankind can move to some suitable exoplanet when needed. However, recent research indicates this not to be the case, since interstellar space is filled with enough ultradense hydrogen H(0) as stable condensed dark matter (Holmlid ...
openaire +2 more sources
Context. The extremely low density of several long-period exoplanets in mature systems is still unexplained - with HIP 41378 f being archetypical of this category. It has been proposed that such planets could actually have normal densities but be surrounded by a ring observed approximately face on, mimicking the transit depth of a puffy planet.
Saillenfest, Melaine +3 more
openaire +3 more sources
Exoplanet weather and climate regimes with clouds and thermal ionospheres
Context. Gaseous exoplanets are the targets that enable us to explore fundamentally our understanding of planetary physics and chemistry. With observational efforts moving from the discovery into the characterisation mode, systematic campaigns that cover
Robin Baeyens +29 more
core +1 more source
Planetary migration and the origin of the 2:1 and 3:2 (near)-resonant population of close-in exoplanets [PDF]
We present an analytical and numerical study of the orbital migration and resonance capture of fictitious two-planet systems with masses in the super-Earth range undergoing Type-I migration. We find that, depending on the flare index and proximity to the central star, the average value of the period ratio, $P_2/P_1$, between both planets may show a ...
Ramos, X. S. +3 more
openaire +4 more sources

