Modelling Spectra of N-Body Simulations of Galaxy Mergers

Details Modelling Spectra of N-Body Simulations of Galaxy Mergers Modelling Spectra of N-Body Simulations of Galaxy Mergers

Jul 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007sf2a.conf..310c&link_type=abstract

SF2A-2007: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics held in Grenoble, France, July

Astronomy and Astrophysics

Astrophysics

Scientific paper

We present an efficient approach to model spectra for N-body simulations of galaxy mergers (Horizon GalMer project) using the PEGASE.HR synthetic populations. Using the pre-computed grid of PEGASE.HR simple stellar populations (SSP) spectra and/or colours, as well as the kinematics of the particles on the line of sight, we are able to make on-the-fly computation of spectra and/or colours for any region of the simulated galaxies as seen from any direction.

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