Galaxy Evolution home
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TelescopesThe group makes extensive use of UK and international telescope facilities.
The analysis of telescope data is done mostly using AIPS, IRAF and STARLINK software which is available throughout the cluster. Additionally we make significant use of IDL for visualisation of results.
Our computational work is concerned both with computational fluid dynamics using mainly the ZEUS family of software (developed at the Laboratory for Computational Astrophysics at the NCSA) and N-body simulations of star-forming galaxies using our owm locally written N-body tree code.
Last modified: 20/1/2002