Photometric evolution of galaxies in rich clusters - Numerical simulations

Details Photometric evolution of galaxies in rich clusters - Numerical simulations Photometric evolution of galaxies in rich clusters - Numerical simulations

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.170..289p&link_type=abstract

(IAU, European Regional Astronomy Meeting, 11th, La Laguna, Spain, July 3-8, 1989) Astrophysics and Space Science (ISSN 0004-640

Astronomy and Astrophysics

Astrophysics

Astronomical Models, Astronomical Photometry, Computerized Simulation, Galactic Clusters, Galactic Evolution, Equations Of Motion, Galactic Bulge, Gravitational Fields, Mass Distribution, Monte Carlo Method, Photochemical Reactions, Stellar Luminosity

Scientific paper

The paper briefly presents a numerical code which simulates the evolution of galaxies belonging to rich clusters. The evolutionary model considers both cluster dynamics and galaxy photometry, taking into account the galaxy-cluster interactions (collisional stripping, merging, and ram-pressure stripping by the ICM) and the intrinsic galaxy evolution. Different initial mass distributions for galaxies are used, and the influence of the initial segregation in mass on the evolution of the photometrical properties is briefly discussed.

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