Modelling the UV to sub-mm SED of starburst galaxies

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dc.contributor.authorDopita, Michael
dc.date.accessioned2015-12-13T22:52:04Z
dc.date.available2015-12-13T22:52:04Z
dc.date.issued2005
dc.date.updated2015-12-11T10:48:53Z
dc.description.abstractThis paper reviews the theoretical modelling of starburst galaxies with particular emphasis on the importance of the gas-phase physics in determining the form of the continuum SED and the emission line spectrum. Both line and continuum diagnostics have been used as star formation indicators. Here, we examine from the point of view of the theory how reliable each of these indicators may be, and to what physics of the galaxy they are sensitive, with the aim of decreasing the errors associated with measuring the star formation history of the universe.
dc.identifier.isbn0735402469
dc.identifier.urihttp://hdl.handle.net/1885/81383
dc.publisherAmerican Institute of Physics (AIP)
dc.relation.ispartofThe Spectral Energy Distributions of Gas-Rich Galaxies: Confronting Models with Data.
dc.relation.isversionof1st Edition
dc.titleModelling the UV to sub-mm SED of starburst galaxies
dc.typeBook chapter
local.bibliographicCitation.lastpage222
local.bibliographicCitation.placeofpublicationMelville, NY
local.bibliographicCitation.startpage203
local.contributor.affiliationDopita, Michael, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidDopita, Michael, u7501303
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationMigratedxPub9684
local.identifier.doi10.1063/1.1913931
local.identifier.scopusID2-s2.0-33746501868
local.type.statusPublished Version

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