Results 61 to 70 of about 70,926 (222)
Emission from Multiple Molecular Isotopologues in a High-inclination Protoplanetary Disk
We present a MIRI-MRS spectrum of the high-inclination protoplanetary disk around the solar-mass (K0) star MY Lup, obtained as part of the JWST Disk Infrared Spectral Chemistry Survey (JDISCS). The spectrum shows an unusually weak water emission spectrum
Colette Salyk+9 more
doaj +1 more source
Structure and evolution of protoplanetary disks [PDF]
We present here a few thoughts on how high-angular resolution observations can give clues to some properties of protoplanetary disks that are fundamental to theories of planet formation.
Apai, Daniel+3 more
core +1 more source
Abstract Calcium‐aluminum‐rich inclusions (CAIs) are the first objects that formed in the solar accretion disk and therefore provide valuable insights into the evolution of the early solar system. A long‐standing question regarding this earliest formative period relates to the storage of CAIs in the 1–4 Myr time period between their formation and later
P. Ghaznavi+3 more
wiley +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
Orbital Evolution of Moons in Weakly Accreting Circumplanetary Disks
We investigate the formation of hot and massive circumplanetary disks (CPDs) and the orbital evolution of satellites formed in these disks. Because of the comparatively small size-scale of the sub-disk, quick magnetic diffusion prevents the ...
Fujii, Yuri I.+3 more
core +1 more source
The Radial Distribution of Dust Particles in the HL Tau Disk from ALMA and VLA Observations [PDF]
Understanding planet formation requires one to discern how dust grows in protoplanetary disks. An important parameter to measure in disks is the maximum dust grain size present.
Anglada, Guillem+15 more
core +3 more sources
Zirconium isotope composition indicates s‐process depletion in samples returned from asteroid Ryugu
Abstract Nucleosynthetic isotope variations are powerful tracers to determine genetic relationships between meteorites and planetary bodies. They can help to link material collected by space missions to known meteorite groups. The Hayabusa 2 mission returned samples from the Cb‐type asteroid (162173) Ryugu.
Maria Schönbächler+89 more
wiley +1 more source
Uncertainties in water chemistry in disks: An application to TW Hya [PDF]
Context. This paper discusses the sensitivity of water lines to chemical processes and radiative transfer for the protoplanetary disk around TW Hya. The study focuses on the Herschel spectral range in the context of new line detections with the PACS ...
Aresu, G.+9 more
core +6 more sources
Evidence for Magnetically‐Driven Accretion in the Distal Solar System
Abstract Paleomagnetic measurements of meteorites indicate that magnetic fields existed in the inner solar nebula capable of driving accretion at rates similar to those observed for young stellar objects with protoplanetary disks. However, the field strength in the solar system beyond ∼7 astronomical units (AU) and its role in accretion remain poorly ...
Elias N. Mansbach+11 more
wiley +1 more source
Exploring the Complex Ionization Environment of the Turbulent DM Tau Disk
Ionization drives important chemical and dynamical processes within protoplanetary disks, including the formation of organics and water in the cold midplane and the transportation of material via accretion and magnetohydrodynamic flows.
Deryl E. Long+11 more
doaj +1 more source