disks. Additionally, I use the physical/chemical modeling code developed at the University of Michigan to investigate the ultimate fate of the missing volatiles under a variety of physical conditions.
Past Work:
Before coming to Michigan I majored in astronomy and physics at the University of Arizona. While there I worked with Professor Yancy Shirley on a project identifying outflows from low mass protostars.
I'm a graduate student at the University of Michigan studying astrochemistry with a focus on protoplanetary disks with Professor Edwin (Ted) Bergin.
Research:
I study the reprocessing of volatile gas phase molecules, such as CO, in protoplanetary disks. With interferometers such as NOEMA and ALMA, I use molecular line emission to constrain the temperature structure and molecular abundances in
office: 406 West Hall
1085 South University Ave.
email: kamberrs at umich dot edu
Astronomy PhD Student, University of Michigan
Huachuca Mountains, Arizona