Speaker
Rob Garrod
(University of Virginia)
Description
I will review the status and results of astrochemical modeling of low-metallicity clouds, including the Magellanic Clouds. A particular emphasis will be placed on the results of grain-surface/ice chemical modeling. I will also present preliminary results from our most recent hot-core chemical models, using metallicities and gas-to-dust ratios appropriate to the outer galaxy. The influence on complex organic molecule abundances in particular will be considered
Primary author
Rob Garrod
(University of Virginia)