University of Hertfordshire

By the same authors

Evolution of the ISM and Galactic Activity

Research output: Contribution to conferencePoster

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  • 0502403

    Accepted author manuscript, 452 KB, PDF-document

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Original languageEnglish
Number of pages6
Publication statusPublished - 1 Feb 2005
Event1st Arizona/Heidelberg Symposium "The High Redshift Frontier" - Tucson, AZ, United States
Duration: 30 Nov 20043 Dec 2004

Conference

Conference1st Arizona/Heidelberg Symposium "The High Redshift Frontier"
CountryUnited States
CityTucson, AZ
Period30/11/043/12/04

Abstract

We study the effects of time-dependent mass injection and heating on the evolution of the interstellar medium (ISM) in elliptical galaxies. As the large and luminous ellipticals have supermassive black holes at their cores, which were probably much less massive in the young universe, feeding these black holes is essential. We examine steady state solutions and describe the impact of the initial starburst on the evolution of the ISM and consequences for galactic activity, based on results from Starburst99.

Notes

Volker Gaibler, Max Camenzind, and Martin Krause, 'Evolution of the ISM and Galactic Activity', paper presented at the 1st Arizona/Heidelberg Symposium "The High Redshift Frontier", 30 November 2004 - 3 December 2004, Tucson, AZ, USA.

ID: 11449361