Results 91 to 100 of about 16,676 (207)
In protoplanetary disks, organic mantle is regarded as promoting the collisional sticking of rocky dust grains. However, the surface energy, which is one of the primary factors determining collisional sticking, has not been well quantified.
Yuuya Nagaashi +2 more
doaj +1 more source
Our understanding of how exoplanets form and evolve relies on analyses of both the mineralogy of protoplanetary disks and their detailed structures; however, these key complementary aspects of disks are usually studied separately.
William Grimble +9 more
doaj +1 more source
JVLA Measurement of Grain Size in the Compact Dust Ring Around Class I Protostar WL 17
The maximum grain size in protoplanetary disks is a critical parameter for planet formation, as the efficiency of mechanisms like streaming instability and pebble accretion depend on grain size.
Jun Hashimoto +4 more
doaj +1 more source
Dead Zones as Thermal Barriers to Rapid Planetary Migration in Protoplanetary Disks
Planetary migration in standard models of gaseous protoplanetary disks is known to be very rapid ($\sim 10^5$ years) jeopardizing the existence of planetary systems.
Baruteau +18 more
core +1 more source
exoALMA. I. Science Goals, Project Design, and Data Products
Planet formation is a hugely dynamic process requiring the transport, concentration, and assimilation of gas and dust to form the first planetesimals and cores.
Richard Teague +40 more
doaj +1 more source
Measuring the Two-dimensional Thermal Structures of Protoplanetary Disks
We present a flexible, annulus-by-annulus method to constrain the 2D thermal structure of a protoplanetary disk from optically thick spectral line emission.
Anna J. Fehr, Sean M. Andrews
doaj +1 more source
Tracing Pebble Drift History in Two Protoplanetary Disks with CO Enhancement
Pebble drift is an important mechanism for supplying the materials needed to build planets in the inner region of protoplanetary disks. Thus, constraining pebble drift’s timescales and mass flux is essential to understanding planet formation history ...
Tayt Armitage +17 more
doaj +1 more source
We present the Atacama Large Millimeter/submillimeter Array Survey of Gas Evolution of PROtoplanetary Disks (AGE-PRO), a large program of the ALMA. AGE-PRO aims to systematically trace the evolution of gas disk mass and size throughout the lifetime of ...
Ke Zhang +21 more
doaj +1 more source
X-ray processing of a realistic ice mantle can explain the gas abundances in protoplanetary disks. [PDF]
Ciaravella A +6 more
europepmc +1 more source
On Kinematic Measurements of Self-gravity in Protoplanetary Disks
Using controlled injection and recovery experiments, we devised an analysis prescription to assess the quality of dynamical measurements of protoplanetary disk gas masses based on resolved (CO) spectral line data, given observational limitations ...
Sean M. Andrews +4 more
doaj +1 more source

