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Dr Stefano Pasetto
Holmbury St. Mary
Dorking
U.K.
Tel: +44 (0)1483 204100
Fax: +44 (0)1483 278312
Appointment
  • Senior Research Associate
  • Dept of Space & Climate Physics
  • Faculty of Maths & Physical Sciences
Biography

Scientific career

2005 March - Ph. D. in Astronomy/Physics, University of Padua (Italy), on “Kinematics of the stellar populations of the Milky Way”, Advisor: Prof. C. Chiosi, Prof. Vallenari, Prof. P. Bertelli

2005 - Post doctoral contract - Astronomy Department of the University of Padua (Padua, Italy) on “The dynamics of the Local Group of Galaxies in cosmological context”, reference Prof. C. Chiosi

2007 - Post doctoral contract - European Association for Research in Astronomy (EARA) grant at the Observatoire de Paris (Paris, France), “The study of the GALMER catalogue”, reference Prof. F. Combes

2007 - External collaboration contract - Institut d’Astrophysique de Paris / Observatoire de Paris (Paris, France) on the “Projection of GALMER”, reference Prof. F. Combes

2007 - Studentship - Max-Planck-Institut für Astronomie and Astronomisches Rechen Institut (Heidelberg, Germany), “The Local Group and our Galaxy”, references Prof. W. Rix & Prof. E.K. Grebel

2009 - Post Doctoral contract - Ruprecht-Karls University Heidelberg (Heidelberg, Germany), “Dynamics of dwarf galaxies in the Local group”, reference Prof. E. K. Grebel

2011 - University College London Research fellow (London, United Kingdom), “Kinematical studies in preparation for Gaia”, reference Prof. M. Cropper

April 2013 till present - Mullard Space Science Laboratory research fellow (London, United Kingdom), “Stellar populations synthesis in preparation for Gaia”, reference Prof. M. Cropper

Research Summary

My research focuses on 

  • energy transfer processes in stellar structure and evolution (convection, radiation, conduction),
  • stellar populations kinematics, dynamics and theory of orbits,
  • dissipative and instability hydro-dynamical processes (Rayleigh–Taylor, Kelvin–Helmholtz, tidal influence,...)

with particular attention to the modelling of our Galaxy’s evolution within the context of the Gaia mission, to the environmental processes on dwarf galaxies of the Local Group and to the star-formation processes and energy-transfer processes (for sun and Supernovae).

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