Results 101 to 110 of about 398,118 (263)
Consistent Dust and Gas Models for Protoplanetary Disks. III. Models for Selected Objects from the FP7 DIANA Project [PDF]
The European FP7 project DIANA has performed a coherent analysis of a large set of observational data of protoplanetary disks by means of thermo-chemical disk models.
P. Woitke +23 more
semanticscholar +1 more source
Abstract We report the discovery of (Al,Cu)‐bearing metallic alloys in two micrometeorites found in the Project Stardust collection gathered from urban rooftop environments in Norway. Most of the alloys are the same as those found in the Khatyrka meteorite and other micrometeorites, though one has a composition that has not been reported previously ...
Luca Bindi +9 more
wiley +1 more source
The inward drift of millimeter–centimeter sized pebbles in protoplanetary disks has become an important part of our current theories of planet formation and, more recently, planet composition as well.
Leon Trapman +18 more
doaj +1 more source
Protoplanetary disks exhibit a vertical gradient in angular momentum, rendering them susceptible to the vertical shear instability (VSI). The most important condition for the onset of this mechanism is a short timescale of thermal relaxation (≲0.1 ...
Thomas Pfeil +2 more
doaj +1 more source
GoFish: Fishing for Line Observations in Protoplanetary Disks
Molecular line observations are an essential complement to high resolution continuum data when studying the planet formation environment, the protoplanetary disk.
R. Teague
semanticscholar +1 more source
Global Simulations of the Inner Regions of Protoplanetary Disks with Comprehensive Disk Microphysics [PDF]
The gas dynamics of weakly ionized protoplanetary disks (PPDs) are largely governed by the coupling between gas and magnetic fields, described by three non-ideal magnetohydrodynamical (MHD) effects (Ohmic, Hall, ambipolar).
X. Bai
semanticscholar +1 more source
An overview of the petrography and petrology of particles from aggregate sample from asteroid Bennu
Abstract The OSIRIS‐REx mission returned a sample of regolith from the carbonaceous asteroid Bennu in September 2023. We present preliminary in situ investigations of the petrology and petrography of selected particles ranging in size from 0.5 to 3 mm.
Harold C. Connolly Jr +57 more
wiley +1 more source
Intermediate mass black holes in AGN disks: I. Production & Growth
Here we propose a mechanism for efficiently growing intermediate mass black holes (IMBH) in disks around supermassive black holes. Stellar mass objects can efficiently agglomerate when facilitated by the gas disk.
Alexander +64 more
core +1 more source
Chemical Richness of protoplanetary Disks and related physical Properties [PDF]
A. Dutrey
openalex +1 more source
Abstract The in‐plane rotation method is used to obtain X‐ray random diffraction (XRD) patterns of polished thin sections of 10 CM chondrites. The samples include five intermediately altered CM chondrites with subtypes 2.6–2.3, two heavily altered CM chondrites with subtype 2.0 and three with secondary heating after hydration (Y 980036, Y 980051, and ...
Naoya Imae +2 more
wiley +1 more source

