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Chemistry in planet-forming regions revealed by ALMA

   Faculty of Engineering and Physical Sciences

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  Dr Catherine Walsh  Applications accepted all year round  Self-Funded PhD Students Only

About the Project

The Atacama Large Millimeter/submillimeter Array (ALMA) is a telescope in Chile that observes the universe at millimeter wavelengths. ALMA has the resolution and sensitivity to observe emission from cold dust and molecular gas on planet-forming scales. This allows us to probe the planet-building environment around nearby stars on size scales similar to the Solar System. Recent observations with ALMA have revealed the almost ubiquitous presence of dust substructure in disks around nearby young stars, in which the dust has been shepherded into concentric dust rings and asymmetric vortices. One of the proposed origins of this dust structure is the presence of still-forming planets within the disk.

A recent ALMA Large Program involving Leeds researchers, titled Molecules with ALMA on Planet-forming Scales or MAPS, imaged for the first time, the chemistry of planet formation on Solar System size scales. These data revealed a wealth of chemical diversity, with observed chemical sub-structure usually not coincident with dust sub-structure. It is still not understood why disks exhibit such chemical diversity but it is likely due to the complex interplay between dust, radiation, chemistry, and transport of material. 

Determining the origin of chemical sub-structure in disks requires the development of new models of protoplanetary disks that incorporate all of these important physical effects. If awarded funding, the successful candidate will develop new models of disk chemistry that include the effects of dust evolution and sub-structure, radial transport, and mixing, motivated by current theories on the origin of dust sub-structure in disks. You will use these models to simulate observations to directly compare with the results from the MAPS ALMA Large Program, and you will produce suites of diagnostics that will be used to motivate future ALMA proposals.

This project would be particularly suited to a candidate interested in conducting a computational project in astrochemistry and planet formation, and who would enjoy the challenge of working with state-of-the-art models and observational data from ALMA. The successful candidate will have a first class or upper second class degree in physics, astrophysics, or astronomy. 

Further information about this project and how to apply can be found on our website.

Funding Notes

This project does not provide funding, but self-funded students may apply.
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