F
Fred J. Ciesla
Researcher at University of Chicago
Publications - 182
Citations - 7466
Fred J. Ciesla is an academic researcher from University of Chicago. The author has contributed to research in topics: Formation and evolution of the Solar System & Protoplanetary disk. The author has an hindex of 46, co-authored 178 publications receiving 6515 citations. Previous affiliations of Fred J. Ciesla include Carnegie Institution for Science & University of Arizona.
Papers
More filters
Journal ArticleDOI
A steeper than linear disk mass-stellar mass scaling relation
Ilaria Pascucci,Leonardo Testi,Leonardo Testi,Gregory J. Herczeg,Feng Long,Carlo F. Manara,Nathanial P. Hendler,Gijs D. Mulders,Sebastiaan Krijt,Fred J. Ciesla,Th. Henning,Subhanjoy Mohanty,Emily Drabek-Maunder,Daniel Apai,László Szűcs,G. G. Sacco,Johan Olofsson +16 more
TL;DR: The Progetti Premiali -iALMA (Progetti-premiali iALMA) project as mentioned in this paper was the first one to use the ALMA project.
Journal ArticleDOI
The evolution of the water distribution in a viscous protoplanetary disk
Fred J. Ciesla,Jeffrey N. Cuzzi +1 more
TL;DR: In this article, the authors present a model which tracks how the distribution of water changes in an evolving disk as the waterbearing species experience condensation, accretion, transport, collisional destruction, and vaporization.
Journal ArticleDOI
A Steeper than Linear Disk Mass-Stellar Mass Scaling Relation
Ilaria Pascucci,Leonardo Testi,Gregory J. Herczeg,Feng Long,Carlo F. Manara,Nathanial P. Hendler,Gijs D. Mulders,Sebastiaan Krijt,Fred J. Ciesla,Th. Henning,Subhanjoy Mohanty,Emily Drabek-Maunder,Daniel Apai,L. Szucs,G. G. Sacco,Johan Olofsson +15 more
TL;DR: In this paper, an ALMA 887micron survey of the disk population around objects from 2 to 0.03Msun in the nearby 2Myr-old Chamaeleon I star-forming region is presented.
Journal ArticleDOI
The Formation Conditions of Chondrules and Chondrites
TL;DR: It is shown that the abundance of the volatile element sodium remained relatively constant during chond rule formation, which explains many other chemical characteristics of chondrules and implies that chondrule and planetesimal formation were linked.
Journal ArticleDOI
Outward Transport of High-Temperature Materials Around the Midplane of the Solar Nebula
TL;DR: A new two-dimensional model shows that outward transport of high-temperature materials in protoplanetary disks is a natural outcome of disk formation and evolution.