From Observations to Self-Consistent Modelling of the ISM in Galaxies

Bibliographic Details
Main Author: de Avillez, Miguel
Publication Date: 2004
Other Authors: Breitschwerdt, Dieter
Format: Book
Language: eng
Source: Repositórios Científicos de Acesso Aberto de Portugal (RCAAP)
Download full: http://hdl.handle.net/10174/5610
Summary: Research of the interstellar medium (ISM) has been advancing rapidly during the last 10 years, mainly due to immensely improved observational facilities and techniques in all wavelength ranges. We are now able to investigate the ISM in external galaxies and even the intergalactic and intracluster medium in great detail. Increased spatial and spectral resolution have provided us with a great deal of information on the interstellar gas in its various phases, the magnetic field and the cosmic rays, and of course, also the stellar component, which is the driving agent of the interstellar matter cycle. Since only fairly recently, a sufficient amount of computing power has become available to tackle these problems with some prospect of obtaining a self-consistent picture of the ISM, a major goal of this workshop was to bring together observers and theoreticians sufficiently close, so that intense discussions about the necessities and desiderata of modelling the ISM could be stimulated. Observers have shown in great detail on this conference of what is seen on all scales of the ISM, near and far, and what boundary conditions would be appropriate for realistic models, and theoreticians pointed out what assumptions and simplifications their codes need, and how future observations could test their models. As a first step towards this goal, some self-consistent numerical simulations with a minimum number of relevant physical processes were also presented on this meeting. There was wide agreement, that this approach - to keep observers and theoreticians in close contact and also in sometimes quite controversial discussions - will bear fruitful results in the near future.
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spelling From Observations to Self-Consistent Modelling of the ISM in GalaxiesInterstellar MediumModellingObservationsGalaxiesResearch of the interstellar medium (ISM) has been advancing rapidly during the last 10 years, mainly due to immensely improved observational facilities and techniques in all wavelength ranges. We are now able to investigate the ISM in external galaxies and even the intergalactic and intracluster medium in great detail. Increased spatial and spectral resolution have provided us with a great deal of information on the interstellar gas in its various phases, the magnetic field and the cosmic rays, and of course, also the stellar component, which is the driving agent of the interstellar matter cycle. Since only fairly recently, a sufficient amount of computing power has become available to tackle these problems with some prospect of obtaining a self-consistent picture of the ISM, a major goal of this workshop was to bring together observers and theoreticians sufficiently close, so that intense discussions about the necessities and desiderata of modelling the ISM could be stimulated. Observers have shown in great detail on this conference of what is seen on all scales of the ISM, near and far, and what boundary conditions would be appropriate for realistic models, and theoreticians pointed out what assumptions and simplifications their codes need, and how future observations could test their models. As a first step towards this goal, some self-consistent numerical simulations with a minimum number of relevant physical processes were also presented on this meeting. There was wide agreement, that this approach - to keep observers and theoreticians in close contact and also in sometimes quite controversial discussions - will bear fruitful results in the near future.Kluwer Academic Publishers2012-11-14T18:08:57Z2012-11-142004-01-01T00:00:00Zinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/bookhttp://hdl.handle.net/10174/5610http://hdl.handle.net/10174/5610eng978-1-4020-1939-5naosimmavillez@galaxy.lca.uevora.ptbreitsch@mpe.mpg.de343de Avillez, MiguelBreitschwerdt, Dieterinfo:eu-repo/semantics/openAccessreponame:Repositórios Científicos de Acesso Aberto de Portugal (RCAAP)instname:FCCN, serviços digitais da FCT – Fundação para a Ciência e a Tecnologiainstacron:RCAAP2024-01-03T18:44:24Zoai:dspace.uevora.pt:10174/5610Portal AgregadorONGhttps://www.rcaap.pt/oai/openaireinfo@rcaap.ptopendoar:https://opendoar.ac.uk/repository/71602025-05-28T11:54:59.200255Repositórios Científicos de Acesso Aberto de Portugal (RCAAP) - FCCN, serviços digitais da FCT – Fundação para a Ciência e a Tecnologiafalse
dc.title.none.fl_str_mv From Observations to Self-Consistent Modelling of the ISM in Galaxies
title From Observations to Self-Consistent Modelling of the ISM in Galaxies
spellingShingle From Observations to Self-Consistent Modelling of the ISM in Galaxies
de Avillez, Miguel
Interstellar Medium
Modelling
Observations
Galaxies
title_short From Observations to Self-Consistent Modelling of the ISM in Galaxies
title_full From Observations to Self-Consistent Modelling of the ISM in Galaxies
title_fullStr From Observations to Self-Consistent Modelling of the ISM in Galaxies
title_full_unstemmed From Observations to Self-Consistent Modelling of the ISM in Galaxies
title_sort From Observations to Self-Consistent Modelling of the ISM in Galaxies
author de Avillez, Miguel
author_facet de Avillez, Miguel
Breitschwerdt, Dieter
author_role author
author2 Breitschwerdt, Dieter
author2_role author
dc.contributor.author.fl_str_mv de Avillez, Miguel
Breitschwerdt, Dieter
dc.subject.por.fl_str_mv Interstellar Medium
Modelling
Observations
Galaxies
topic Interstellar Medium
Modelling
Observations
Galaxies
description Research of the interstellar medium (ISM) has been advancing rapidly during the last 10 years, mainly due to immensely improved observational facilities and techniques in all wavelength ranges. We are now able to investigate the ISM in external galaxies and even the intergalactic and intracluster medium in great detail. Increased spatial and spectral resolution have provided us with a great deal of information on the interstellar gas in its various phases, the magnetic field and the cosmic rays, and of course, also the stellar component, which is the driving agent of the interstellar matter cycle. Since only fairly recently, a sufficient amount of computing power has become available to tackle these problems with some prospect of obtaining a self-consistent picture of the ISM, a major goal of this workshop was to bring together observers and theoreticians sufficiently close, so that intense discussions about the necessities and desiderata of modelling the ISM could be stimulated. Observers have shown in great detail on this conference of what is seen on all scales of the ISM, near and far, and what boundary conditions would be appropriate for realistic models, and theoreticians pointed out what assumptions and simplifications their codes need, and how future observations could test their models. As a first step towards this goal, some self-consistent numerical simulations with a minimum number of relevant physical processes were also presented on this meeting. There was wide agreement, that this approach - to keep observers and theoreticians in close contact and also in sometimes quite controversial discussions - will bear fruitful results in the near future.
publishDate 2004
dc.date.none.fl_str_mv 2004-01-01T00:00:00Z
2012-11-14T18:08:57Z
2012-11-14
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
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dc.identifier.uri.fl_str_mv http://hdl.handle.net/10174/5610
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url http://hdl.handle.net/10174/5610
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv 978-1-4020-1939-5
nao
sim
mavillez@galaxy.lca.uevora.pt
breitsch@mpe.mpg.de
343
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