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Astrophysics Luncheon Seminar

Protoplanetary Disk Masses in Taurus and the Orion Nebula Cluster
Presented by Nick Ballering
Steward Observatory, University of Arizona

Monday, October 1, 2018
12:00 noon in 169-336

The masses of protoplanetary disks are a primary factor influencing the efficiency of planet formation. I will present the results of fitting radiative transfer models to the spectral energy distributions of disks in the Taurus star-forming region. Such models can provide a more accurate determination of disk masses than (sub-)mm photometry alone, while offering insight into the assumptions that are often employed when measuring disk masses. I will also highlight the results of our recent ALMA observations of disks in the Orion Nebula Cluster which reveal the effects of the cluster environment on disk properties.

JPL Contact: Karl Stapelfeldt (4-9608)

About the Speaker
Nick is interested in planet formation and circumstellar disks. He earned a PhD at the University of Arizona working with George Rieke to study the structure and composition of debris disks. He is currently a postdoc at the University of Arizona working with Josh Eisner to measure the masses of protoplanetary disks in various star forming environments

SVCP Astrophysics

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