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dc.contributor.authorGaibler, V.
dc.contributor.authorCamenzind, M.
dc.contributor.authorKrause, M.
dc.date.accessioned2017-04-19T14:16:45Z
dc.date.available2017-04-19T14:16:45Z
dc.date.issued2005-02-01
dc.identifier.citationGaibler , V , Camenzind , M & Krause , M 2005 , ' Evolution of the ISM and Galactic Activity ' , 1st Arizona/Heidelberg Symposium "The High Redshift Frontier" , Tucson, AZ , United States , 30/11/04 - 3/12/04 . < https://arxiv.org/pdf/astro-ph/0502403v1.pdf >
dc.identifier.citationconference
dc.identifier.otherBibtex: urn:83dadbf4ee51b5bb71c6221884624810
dc.identifier.otherORCID: /0000-0002-9610-5629/work/63687408
dc.identifier.urihttp://hdl.handle.net/2299/17971
dc.descriptionVolker 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.
dc.description.abstractWe 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.en
dc.format.extent6
dc.format.extent463297
dc.language.isoeng
dc.titleEvolution of the ISM and Galactic Activityen
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.contributor.institutionDepartment of Physics, Astronomy and Mathematics
dc.description.statusNon peer reviewed
dc.identifier.urlhttps://arxiv.org/pdf/astro-ph/0502403v1.pdf
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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