Don't miss our weekly PhD newsletter | Sign up now Don't miss our weekly PhD newsletter | Sign up now

  Dust and molecules in core-collapse supernovae (astronomy)


   Cardiff School of Physics and Astronomy

This project is no longer listed on FindAPhD.com and may not be available.

Click here to search FindAPhD.com for PhD studentship opportunities
  Dr M Matsuura  No more applications being accepted  Competition Funded PhD Project (European/UK Students Only)

About the Project

Explosions of supernovae eject newly synthesised elements into the interstellar medium, making supernovae the key for enriching interstellar medium of heavy elements. Yet, it is not well measured how much elements are synthesised and in what state they form.
Recently, the Herschel Space Observatory and ALMA discovered that majority of heavy elements can turn into dust and molecules. The PhD student will exploit the Herschel and ALMA data, with modelling their thermal emissions and molecular spectra. They will reveal quantity of molecules and dust, as well as the dynamics of supernovae, using molecular lines as a probe.

Funding Notes

This project is available to students applying for funded PhD studentships and may be altered or amended.
Studentships will be awarded to successful applicants from all applications received. Applicants must satisfy RCUK residency rules for the full studentship.

How good is research at Cardiff University in Physics?


Research output data provided by the Research Excellence Framework (REF)

Click here to see the results for all UK universities

Where will I study?