Results 101 to 110 of about 5,108 (182)
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
Shadow-induced Warps in Protoplanetary Disks
Shadows are commonly observed in protoplanetary disks in near-infrared (NIR) and (sub)millimeter images, often cast by misaligned inner disks or other obscuring material.
Shangjia Zhang +2 more
doaj +1 more source
Gas in Protoplanetary and Debris Disks: Insights from UV Spectroscopy [PDF]
Over the last two decades, observations of protoplanetary and debris disks have played an important role in the new field of extrasolar planetary studies.
Roberge, Aki
core
Current imaging observations of protoplanetary disks using the Atacama Large Millimeter/submillimeter Array (ALMA) primarily focus on the submillimeter wavelength, leaving a gap in effective observational approaches for centimeter-sized dust, which is ...
Yinhao Wu +3 more
doaj +1 more source
Context. Protoplanetary disk substructures are thought to play a crucial role in disk evolution and planet formation. Population studies of disks large-sample size surveys show that not only substructure, but also their rapid formation, are needed to ...
Delussu Luca +7 more
doaj +1 more source
Substructures of Protoplanetary Disks Revealed with ALMA Radio Observations [PDF]
Protoplanetary disks, the birth places of planets, are rotating disks of dust and gas surrounding still-forming stars. Studying the lifetime, mass, size, structure, and compositions of protoplanetary disks through observations at infrared or millimeter ...
Dong, Jiayin
core
SO Emission in the Dynamically Perturbed Protoplanetary Disks around CQ Tau and MWC 758
We report the serendipitous detection of the SO J _N = 6 _5 –5 _4 (219.949 GHz) rotational transition in archival Atacama Large Millimeter/submillimeter Array observations of the spiral hosting protoplanetary disks around CQ Tau (with ≈4.9 σ ...
Francesco Zagaria +27 more
doaj +1 more source
On the Interpretation of Velocity Residuals in Protoplanetary Disks
We present a first-order analytical model for line-of-sight velocity residuals, defined as the difference between observed velocities and those predicted by a fiducial model, assuming a flared, nearly axisymmetric disk with the perturbations in disk ...
Masataka Aizawa, Ryuta Orihara
doaj +1 more source
<i>Herschel</i> survey and modelling of externally-illuminated photoevaporating protoplanetary disks. [PDF]
Champion J +7 more
europepmc +1 more source
exoALMA. XXI. The Morphology and Dynamics of Vertical Flows
Vertical gas flows—such as winds and meridional circulations—are natural outcomes of protoplanetary disk processes and play a critical role in the earliest stages of planet formation.
Myriam Benisty +35 more
doaj +1 more source

