I am currently a graduate student working on a PhD in Physics at the University of California Santa Cruz. I study the formation and evolution of galaxies with my thesis advisor Joel Primack and collaborators T.J. Cox, Avishai Dekel, and Patrik Jonsson. My research uses a large set of hydrodynamical galaxy merger simulations as a test bed for constructing simple, physically-based models for the processes that occur during galaxy mergers. More recently, I have been extending this work to examine comparisions between the simulations and observed galaxies in collaboration with AEGIS.

My research areas of interest include:

  • models of galaxy mergers
  • origin and evolution of the fundamental scaling relations of galaxies
  • fueling of Active Galactic Nuclei
  • dynamical friction and orbits of satellite dark matter halos
  • understanding the roles of hydrodynamics and feedback in galaxy formation

Matt Covington
NSF International
Research Fellow


Address:
Karst Research Institute
Titov Trg 2
6230 Postojna
Slovenia

email:
speleophysics at gmail
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