Linking planetesimal and dust content in protoplanetary disks via a local toy model [PDF]
Konstantin Gerbig +2 more
openalex +1 more source
SMA and NOEMA Reveal Asymmetric Substructure in the Protoplanetary Disk of IRAS 23077+6707
We present high-resolution data of IRAS 23077+6707 (“ Dracula’s Chivito ”) with the Submillimeter Array (SMA at 1.33 mm/225.5 GHz) and the Northern Extended Millimeter Array (NOEMA at 2.7 mm/111.7 GHz and 3.1 mm/96.2 GHz).
Joshua B. Lovell +7 more
doaj +1 more source
Dust-driven viscous ring-instability in protoplanetary disks
Protoplanetary disks often appear as multiple concentric rings in dust continuum emission maps and scattered light images. These features are often associated with possible young planets in these disks.
Dullemond, C. P., Penzlin, A. B. T.
core +1 more source
Light Echoes of Time-resolved Flares and Application to Kepler Data
Light echoes of stellar flares provide an intriguing option for exploring protoplanetary disks in young stellar systems. Previous work on light echoes of circumstellar disks made use of delta-function flares for modeling.
Austin King, Benjamin C. Bromley
doaj +1 more source
The Meteoritical Society: Business from 2023 to 2024
Meteoritics &Planetary Science, Volume 60, Issue 3, Page 680-696, March 2025.
Nancy L. Chabot +2 more
wiley +1 more source
THE MAGNETIC FIELD IMPACT ON ACCRETION RATE IN A PROTOPLANETARY DISK
Recent observations are the evidence of a large-scale magnetic field in discs around classical T Tauri stars. A model of the axisymmetric thin protoplanetary disk in a global magnetic field is considered.
M. M. Kuksa
doaj +1 more source
Observations of edge-on protoplanetary disks with ALMA I. Results from continuum data [PDF]
M. Villenave +17 more
openalex +1 more source
Growing and trapping pebbles with fragile collisions of particles in protoplanetary disks [PDF]
Paola Pinilla +2 more
openalex +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
Monte Carlo simulation of sugar synthesis on icy dust particles intermittently irradiated by UV in a protoplanetary disk [PDF]
Hitoshi Takehara +2 more
openalex +1 more source

