Research output: Contribution to conference › Poster
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| Original language | English |
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| Number of pages | 6 |
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| Publication status | Published - 1 Feb 2005 |
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| Event | 1st Arizona/Heidelberg Symposium "The High Redshift Frontier" - Tucson, AZ, United States
Duration: 30 Nov 2004 → 3 Dec 2004 |
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| Conference | 1st Arizona/Heidelberg Symposium "The High Redshift Frontier" |
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| Country/Territory | United States |
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| City | Tucson, AZ |
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| Period | 30/11/04 → 3/12/04 |
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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