Results 131 to 140 of about 71,588 (268)
On the Submillimeter Opacity of Protoplanetary Disks [PDF]
Submitted to ApJ.
openaire +3 more sources
Carbon isotope fractionation in protoplanetary disks
We investigate the gas-phase and grain-surface chemistry in the inner 30 AU of a typical protoplanetary disk using a new model which calculates the gas temperature by solving the gas heating and cooling balance and which has an improved treatment of the ...
Aikawa+75 more
core +1 more source
We present James Webb Space Telescope imaging from 2 to 21 μ m of the edge-on protoplanetary disk around the embedded young star IRAS04302+2247. The structure of the source shows two reflection nebulae separated by a dark lane.
Marion Villenave+8 more
doaj +1 more source
We present a mid-IR interferometric survey of the circumstellar environment of a specific class of post-Asymptotic Giant Branch (post-AGB) binaries. For this class the presence of a compact dusty disk has been postulated on the basis of various spatially
de Wit, W. -J.+9 more
core +1 more source
Planet Formation Regulated by Galactic-scale Interstellar Turbulence
Planet formation occurs over a few Myr within protoplanetary disks of dust and gas, which are often assumed to evolve in isolation. However, extended gaseous structures have been uncovered around many protoplanetary disks, suggestive of late-stage infall
Andrew J. Winter+2 more
doaj +1 more source
The Short Circuit Instability in Protoplanetary Disks: Processing high temperature minerals
We introduce a magneto-hydrodynamic instability which occurs, among other locations, in the inner, hot regions of protoplanetary disks, and which alters the way in which resistive dissipation of magnetic energy into heat proceeds.
D’Alessio P.+4 more
doaj +1 more source
Evolution of the Solar Nebula. III. Protoplanetary Disks Undergoing Mass Accretion [PDF]
Alan P. Boss
openalex +1 more source
Magnetic fields of protoplanetary disks [PDF]
We review the current status of studies on accretion and protoplanetary disks of young stars with large-scale magnetic fields. Observational data on magnetic fields of the disks are compiled and analysed. Modern analytical and numerical MHD models of protoplanetary disks are discussed.
arxiv
On rapid migration and accretion within disks around supermassive black holes
Galactic nuclei should contain a cluster of stars and compact objects in the vicinity of the central supermassive black hole due to stellar evolution, minor mergers and gravitational dynamical friction.
Alexander+50 more
core +1 more source