Evolution of star-forming dwarf galaxies: characterizing the star formation scenarios

We use the self-consistent model technique developed by Martín-Manjón et al. That combines the chemical evolution with stellar population synthesis and photoionization codes, to study the star formation scenarios capable of reproducing the observed properties of star-forming galaxies. The comparison...

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Detalles Bibliográficos
Autor: ROBERTO GIOVANNI TERLEVICH
Tipo de recurso: artículo
Estado:Versión aceptada para publicación
Fecha de publicación:2012
País:México
Institución:Instituto Nacional de Astrofísica, Óptica y Electrónica
Repositorio:Repositorio Institucional del INAOE
Idioma:inglés
OAI Identifier:oai:inaoe.repositorioinstitucional.mx:1009/1861
Acceso en línea:http://inaoe.repositorioinstitucional.mx/jspui/handle/1009/1861
Access Level:acceso abierto
Palabra clave:info:eu-repo/classification/Inspec/HII regions
info:eu-repo/classification/Inspec/Galaxies: dwarf
info:eu-repo/classification/Inspec/Galaxies: evolution
info:eu-repo/classification/Inspec/Galaxies: ISM
info:eu-repo/classification/Inspec/Galaxies: starburst
info:eu-repo/classification/Inspec/Galaxies: star formation
info:eu-repo/classification/cti/1
info:eu-repo/classification/cti/21
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network_acronym_str MX
network_name_str México
repository_id_str
spelling Evolution of star-forming dwarf galaxies: characterizing the star formation scenariosROBERTO GIOVANNI TERLEVICHinfo:eu-repo/classification/Inspec/HII regionsinfo:eu-repo/classification/Inspec/Galaxies: dwarfinfo:eu-repo/classification/Inspec/Galaxies: evolutioninfo:eu-repo/classification/Inspec/Galaxies: ISMinfo:eu-repo/classification/Inspec/Galaxies: starburstinfo:eu-repo/classification/Inspec/Galaxies: star formationinfo:eu-repo/classification/cti/1info:eu-repo/classification/cti/21info:eu-repo/classification/cti/21We use the self-consistent model technique developed by Martín-Manjón et al. That combines the chemical evolution with stellar population synthesis and photoionization codes, to study the star formation scenarios capable of reproducing the observed properties of star-forming galaxies. The comparison of our model results with a data base of HII galaxies shows that the observed spectra and colours of the present burst and the older underlying population are reproduced by models in a bursting scenario with star formation efficiency involving close to 20 per cent of the total mass of gas, and interburst times longer than 100 Myr, and more probably around 1 Gyr. Other modes like gasping and continuous star formation are not favoured.Monthly Notices of the Royal Astronomical Society2012-02info:eu-repo/semantics/articleinfo:eu-repo/semantics/acceptedVersionapplication/pdfhttp://inaoe.repositorioinstitucional.mx/jspui/handle/1009/1861reponame:Repositorio Institucional del INAOEinstname:Instituto Nacional de Astrofísica, Óptica y Electrónicainstacron:INAOEengcitation:Martín Manjón, M. L., et al., (2012), Evolution of star-forming dwarf galaxies: characterizing the star formation scenarios, Monthly Notices of the Royal Astronomical Society, Vol. 420(2):1294–1308info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-nd/4.0oai:inaoe.repositorioinstitucional.mx:1009/18612024-08-28T03:23:01Z
dc.title.none.fl_str_mv Evolution of star-forming dwarf galaxies: characterizing the star formation scenarios
title Evolution of star-forming dwarf galaxies: characterizing the star formation scenarios
spellingShingle Evolution of star-forming dwarf galaxies: characterizing the star formation scenarios
ROBERTO GIOVANNI TERLEVICH
info:eu-repo/classification/Inspec/HII regions
info:eu-repo/classification/Inspec/Galaxies: dwarf
info:eu-repo/classification/Inspec/Galaxies: evolution
info:eu-repo/classification/Inspec/Galaxies: ISM
info:eu-repo/classification/Inspec/Galaxies: starburst
info:eu-repo/classification/Inspec/Galaxies: star formation
info:eu-repo/classification/cti/1
info:eu-repo/classification/cti/21
info:eu-repo/classification/cti/21
title_short Evolution of star-forming dwarf galaxies: characterizing the star formation scenarios
title_full Evolution of star-forming dwarf galaxies: characterizing the star formation scenarios
title_fullStr Evolution of star-forming dwarf galaxies: characterizing the star formation scenarios
title_full_unstemmed Evolution of star-forming dwarf galaxies: characterizing the star formation scenarios
title_sort Evolution of star-forming dwarf galaxies: characterizing the star formation scenarios
dc.creator.none.fl_str_mv ROBERTO GIOVANNI TERLEVICH
author ROBERTO GIOVANNI TERLEVICH
author_facet ROBERTO GIOVANNI TERLEVICH
author_role author
dc.subject.none.fl_str_mv info:eu-repo/classification/Inspec/HII regions
info:eu-repo/classification/Inspec/Galaxies: dwarf
info:eu-repo/classification/Inspec/Galaxies: evolution
info:eu-repo/classification/Inspec/Galaxies: ISM
info:eu-repo/classification/Inspec/Galaxies: starburst
info:eu-repo/classification/Inspec/Galaxies: star formation
info:eu-repo/classification/cti/1
info:eu-repo/classification/cti/21
info:eu-repo/classification/cti/21
topic info:eu-repo/classification/Inspec/HII regions
info:eu-repo/classification/Inspec/Galaxies: dwarf
info:eu-repo/classification/Inspec/Galaxies: evolution
info:eu-repo/classification/Inspec/Galaxies: ISM
info:eu-repo/classification/Inspec/Galaxies: starburst
info:eu-repo/classification/Inspec/Galaxies: star formation
info:eu-repo/classification/cti/1
info:eu-repo/classification/cti/21
info:eu-repo/classification/cti/21
description We use the self-consistent model technique developed by Martín-Manjón et al. That combines the chemical evolution with stellar population synthesis and photoionization codes, to study the star formation scenarios capable of reproducing the observed properties of star-forming galaxies. The comparison of our model results with a data base of HII galaxies shows that the observed spectra and colours of the present burst and the older underlying population are reproduced by models in a bursting scenario with star formation efficiency involving close to 20 per cent of the total mass of gas, and interburst times longer than 100 Myr, and more probably around 1 Gyr. Other modes like gasping and continuous star formation are not favoured.
publishDate 2012
dc.date.none.fl_str_mv 2012-02
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/acceptedVersion
format article
status_str acceptedVersion
dc.identifier.none.fl_str_mv http://inaoe.repositorioinstitucional.mx/jspui/handle/1009/1861
url http://inaoe.repositorioinstitucional.mx/jspui/handle/1009/1861
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv citation:Martín Manjón, M. L., et al., (2012), Evolution of star-forming dwarf galaxies: characterizing the star formation scenarios, Monthly Notices of the Royal Astronomical Society, Vol. 420(2):1294–1308
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
http://creativecommons.org/licenses/by-nc-nd/4.0
eu_rights_str_mv openAccess
rights_invalid_str_mv http://creativecommons.org/licenses/by-nc-nd/4.0
dc.format.none.fl_str_mv application/pdf
dc.publisher.none.fl_str_mv Monthly Notices of the Royal Astronomical Society
publisher.none.fl_str_mv Monthly Notices of the Royal Astronomical Society
dc.source.none.fl_str_mv reponame:Repositorio Institucional del INAOE
instname:Instituto Nacional de Astrofísica, Óptica y Electrónica
instacron:INAOE
instname_str Instituto Nacional de Astrofísica, Óptica y Electrónica
instacron_str INAOE
institution INAOE
reponame_str Repositorio Institucional del INAOE
collection Repositorio Institucional del INAOE
repository.name.fl_str_mv
repository.mail.fl_str_mv
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score 15,198674

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