Results 111 to 120 of about 22,425 (264)
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
Molecules with ALMA at Planet-forming Scales (MAPS). XII. Inferring the C/O and S/H Ratios in Protoplanetary Disks with Sulfur Molecules [PDF]
Romane Le Gal +26 more
openalex +1 more source
Oxygen Isotope Constraints on the Importance of Photochemical Processing in Protoplanetary Disks
Observations have revealed evidence of photochemical processing in protoplanetary disks. This processing occurs in the photon-dominated layer, the optically thin regions of the disk high above the disk midplane. It remains unclear, however, how much this
Fred J. Ciesla +3 more
doaj +1 more source
Dust Evolution in Protoplanetary Disks
Submitted version, to be published in: Handbook of Exoplanets, 2nd Edition, Hans Deeg and Juan Antonio Belmonte (Eds. in Chief), Springer International Publishing AG, part of Springer Nature. Comments welcome.
van der Marel, Nienke, Pinilla, Paola
openaire +2 more sources
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
Protoplanetary Disk Sizes and Angular Momentum Transport [PDF]
Joan Najita, Edwin A. Bergin
openalex +1 more source
87th Annual Meeting of the Meteoritical Society 2025: Contents
Meteoritics &Planetary Science, Volume 60, Issue S1, Page 2-29, August 2025.
wiley +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
Chondrules reveal large-scale outward transport of inner Solar System materials in the protoplanetary disk. [PDF]
Williams CD +7 more
europepmc +1 more source

