Infrared emission lines in the dusty interstellar medium
Elijah Kane, Observational Cosmology / Caltech
Infrared emission lines are powerful probes of the physical conditions within dust-obscured regions, such as protoplanetary disks, molecular clouds, and active galactic nuclei. In this talk I will describe the physics behind this line emission and show examples of how measurements of atomic and molecular lines have been used to help us understand the dusty ISM.
Host: Rui
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