Modelling the Galaxy for GAIA

Techniques for the construction of dynamical Galaxy models should be considered essential infrastructure that should be put in place before GAIA flies. Three possible modelling techniques are discussed. Although one of these seems to have significantly more potential than the other two, at this stag...

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Main Author: Binney, J
Format: Journal article
Published: 2004
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author Binney, J
author_facet Binney, J
author_sort Binney, J
collection OXFORD
description Techniques for the construction of dynamical Galaxy models should be considered essential infrastructure that should be put in place before GAIA flies. Three possible modelling techniques are discussed. Although one of these seems to have significantly more potential than the other two, at this stage work should be done on all three. A major effort is needed to decide how to make a model consistent with a catalogue such as that which GAIA will produce. Given the complexity of the problem, it is argued that a hierarchy of models should be constructed, of ever increasing complexity and quality of fit to the data. The potential that resonances and tidal streams have to indicate how a model should be refined is briefly discussed.
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spelling oxford-uuid:f080542f-81a7-4afe-bb3c-b4e0e630fff82022-03-27T11:48:23ZModelling the Galaxy for GAIAJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:f080542f-81a7-4afe-bb3c-b4e0e630fff8Symplectic Elements at Oxford2004Binney, JTechniques for the construction of dynamical Galaxy models should be considered essential infrastructure that should be put in place before GAIA flies. Three possible modelling techniques are discussed. Although one of these seems to have significantly more potential than the other two, at this stage work should be done on all three. A major effort is needed to decide how to make a model consistent with a catalogue such as that which GAIA will produce. Given the complexity of the problem, it is argued that a hierarchy of models should be constructed, of ever increasing complexity and quality of fit to the data. The potential that resonances and tidal streams have to indicate how a model should be refined is briefly discussed.
spellingShingle Binney, J
Modelling the Galaxy for GAIA
title Modelling the Galaxy for GAIA
title_full Modelling the Galaxy for GAIA
title_fullStr Modelling the Galaxy for GAIA
title_full_unstemmed Modelling the Galaxy for GAIA
title_short Modelling the Galaxy for GAIA
title_sort modelling the galaxy for gaia
work_keys_str_mv AT binneyj modellingthegalaxyforgaia