Hostname: page-component-7bb8b95d7b-s9k8s Total loading time: 0 Render date: 2024-09-27T22:44:16.098Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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