Results 141 to 150 of about 11,561 (252)
Debris disks or exo-Kuiper belts, detected through their thermal or scattered emission from their dusty components, are ubiquitous around main-sequence stars.
Antranik A. Sefilian
doaj +1 more source
Limits on orbit-crossing planetesimals in the resonant multiple planet system, KOI-730 [PDF]
Alexander Moore +2 more
openalex +1 more source
Motion of Planetesimals in the Hill Sphere of the Star Proxima Centauri
С. И. Ипатов
openalex +2 more sources
Convective Overstability in Radially Global Protoplanetary Disks. I. Pure Gas Dynamics
Protoplanetary disks are prone to several hydrodynamic instabilities. One candidate, convective overstability (COS), can drive radial semiconvection that may influence dust dynamics and planetesimal formation.
Marius Lehmann, Min-Kai Lin
doaj +1 more source
Possible Ribose Synthesis in Carbonaceous Planetesimals. [PDF]
Paschek K +7 more
europepmc +1 more source
Implications of the interstellar object 1I/'Oumuamua for planetary dynamics and planetesimal formation [PDF]
Sean N. Raymond +4 more
openalex +1 more source
No evidence for a strong decrease of planetesimal accretion in old white dwarfs [PDF]
Simon Blouin, Siyi Xu
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ON THE FEEDING ZONE OF PLANETESIMAL FORMATION BY THE STREAMING INSTABILITY [PDF]
Chao‐Chin Yang, Anders Johansen
openalex +1 more source
Distinguishing the Origin of Asteroid (16) Psyche. [PDF]
Elkins-Tanton LT +21 more
europepmc +1 more source
Being one of the most populated mean motion resonances (MMRs) with Neptune and lying close to the inner boundary of the present-day cold classical disk, observations of the orbital and surface class distributions of the plutinos in the 3:2 MMR provide ...
Cameron Collyer +8 more
doaj +1 more source

