|CCP7 is a Collaborative
Computational Project, financed by the Particle Physics and Astronomy Research
of the UK. It is concerned with the calculation of theoretical models suitable for the
interpretation of stellar and interstellar spectra. It aims to:
This site has a mirror at STScI in America.
On 19th January 2000 postscript file of the paper "The cooling of astrophysical media by HD" by D.R. Flower et al has been added to Publications.
On 27th October 2000 postscript file of the paper "Sputtering of grains in C-type shocks" by P.W. May et al has been added to Publications.
On 26th February 2001, data pertaining to the paper "Collisional excitation of H2 by grains in C-type shocks" by G. Pineau des ForÍts et al has been added to Publications.
On 7th June 2001, data pertaining to the paper "The rotational excitation of CO by H2" by D.R. Flower has been added to Publications.
Disclaimer: CCP7 software has mostly been donated by third party authors, often on a collaborative basis. Whilst every effort is made to keep software current, limited resources mean that more recent revisions may exist elsewhere. Therefore CCP7 can accept no responsibility for loss or damage incurred by the use of software or any other advice or information obtained through these pages.