455 citations · 914 across the 7 of their papers we have counts for
7 papers
A Steeper than Linear Disk Mass-Stellar Mass Scaling Relation
I. Pascucci, L. Testi, G. J. Herczeg +13
The disk mass is among the most important input parameter for every planet formation model to determine the number and masses of the planets that can form. We present an ALMA 887mi…
Direct imaging of the water snow line at the time of planet formation using two ALMA continuum bands
Andrea Banzatti, Paola Pinilla, Luca Ricci +3
Molecular snow lines in protoplanetary disks have been studied theoretically for decades because of their importance in shaping planetary architectures and compositions. The water…
The early impact histories of meteorite parent bodies
Thomas M Davison, David P O'Brien, Fred J Ciesla +1
We have developed a statistical framework that uses collisional evolution models, shock physics modeling and scaling laws to determine the range of plausible collisional histories…
Residence Times of Particles in Diffusive Protoplanetary Disk Environments II. Radial Motions and Applications to Dust Annealing
Fred J. Ciesla
The origin of crystalline grains in comets and the outer regions of protoplanetary disks remains a mystery. It has been suggested that such grains form via annealing of amorphous p…
Heterogeneous distribution of Al-26 at the birth of the Solar System
Kentaro Makide, Kazuhide Nagashima, Alexander N. Krot +5
It is believed that Al-26, a short-lived (t1/2 = 0.73 Ma) and now extinct radionuclide, was uniformly distributed in the nascent Solar System with the initial Al-26/Al-27 ratio of…
Residence Times of Particles in Diffusive Protoplanetary Disk Environments I. Vertical Motions
Fred J. Ciesla
The chemical and physical evolution of primitive materials in protoplanetary disks are determined by the types of environments they are exposed to and their residence times within…