Current time at conference location: 3:47 pm CT
Session ID
239
Summary
Several large science programs are using the Green Bank Telescope to study a plethora of physical properties, dynamics, and chemistry within the ISM and star-forming molecular clouds. These programs range from observations of the diffuse ionized ISM to studying the kinematics of dense molecular gas cores and cover frequencies from 300 MHz to 115 GHz, leveraging the full capabilities of the GBT. The goal of this special session is to bring together these science teams to highlight recent science results and to demonstrate the collective power of the surveys in addressing the complex physical processes and chemistry within the ISM associated with star formation within our Galaxy and nearby galaxies.

Dynamics in Star-forming Cores (DiSCo): A first look at the internal velocity structures of Perseus star-forming cores with Argus

2:48 PM CT - 3:00 PM CT
Program Number: 239.05
Rachel Friesen, Universtiy of Toronto; Che-Yu Chen, Lawrence Livermore National Laboratory; Jialu Li, University of Maryland; Anika Schmiedeke, Green Bank Observatory; David Frayer, Green Bank Observatory; DiSCo.