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Models of emission line regions around central cluster galaxies

Published online by Cambridge University Press:  07 August 2017

A. C. S. Friaça
A. C. S. Friaça*
Affiliation:
Instituto Astronômico e Geofísico - U.S.P. C.P. 9638, 01065 SÃo Paulo, S.P. - Brasil

Abstract

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Hydrodynamical time-dependent models allows to follow the evolution of condensations in cooling flows until the phase of optical line emission.

References

Friaça, A.C.S. 1991, A. & A. , submitted.Google Scholar
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Viegas-Aldrovandi, S.M., and Contini, M. 1989, A.& A. , 215, 253.Google Scholar