Evolution of the ISM and Galactic Activity

V. Gaibler; M. Camenzind; M. Krause

Evolution of the ISM and Galactic Activity

V. Gaibler, M. Camenzind, M. Krause

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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.

Original language	English
Number of pages	6
Publication status	Published - 1 Feb 2005
Event	1st Arizona/Heidelberg Symposium "The High Redshift Frontier" - Tucson, AZ, United States Duration: 30 Nov 2004 → 3 Dec 2004

Conference

Conference	1st Arizona/Heidelberg Symposium "The High Redshift Frontier"
Country/Territory	United States
City	Tucson, AZ
Period	30/11/04 → 3/12/04

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0502403Accepted author manuscript, 452 KB

https://arxiv.org/pdf/astro-ph/0502403v1.pdf

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title = "Evolution of the ISM and Galactic Activity",

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.",

author = "V. Gaibler and M. Camenzind and M. Krause",

note = "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. ; 1st Arizona/Heidelberg Symposium {"}The High Redshift Frontier{"} ; Conference date: 30-11-2004 Through 03-12-2004",

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T1 - Evolution of the ISM and Galactic Activity

AU - Gaibler, V.

AU - Camenzind, M.

AU - Krause, M.

N1 - 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.

PY - 2005/2/1

Y1 - 2005/2/1

N2 - 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.

AB - 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.

M3 - Poster

T2 - 1st Arizona/Heidelberg Symposium "The High Redshift Frontier"

Y2 - 30 November 2004 through 3 December 2004

ER -

Evolution of the ISM and Galactic Activity

Abstract

Conference

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