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Chemodynamic and Photometric Evolution of Elliptical Galaxies

Published online by Cambridge University Press:  07 August 2017

J. Loxen ,
U. Fritze-V. Alvensleben ,
K.J. Fricke  and
G. Hensler
J. Loxen
Affiliation:
Universitäts-Sternwarte Göttingen, Geismarlandstraße 11, 37083 Göttingen
U. Fritze-V. Alvensleben
Affiliation:
Universitäts-Sternwarte Göttingen, Geismarlandstraße 11, 37083 Göttingen
K.J. Fricke
Affiliation:
Universitäts-Sternwarte Göttingen, Geismarlandstraße 11, 37083 Göttingen
G. Hensler
Affiliation:
Universitätssternwarte Kiel, Olshausenstraße 40, 24118 Kiel

Extract

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In many hydrodynamical models of elliptical galaxies the absence of information about the detailed evolution of stars and the spectro-photometric output by hot gas and stars leads to a missing link between the data we obtain in observations (photons) and the internal behavior (dynamics) of a galaxy.

Type
Poster Papers
Information
Symposium - International Astronomical Union , Volume 164: Stellar Populations , 1995 , pp. 440
Copyright
Copyright © Kluwer 1995