Dust obscuration in starburst galaxies from near-infrared spectroscopy

Detalhes bibliográficos
Autor(a) principal: Calzetti, Daniela
Data de Publicação: 1996
Outros Autores: Kinney, Anne Louise, Storchi-Bergmann, Thaisa
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UFRGS
Texto Completo: http://hdl.handle.net/10183/108780
Resumo: We present new observations of the near-infrared hydrogen recombination lines Paβ and Bry in the central starburst regions of 13 galaxies. The near-infrared data are supplemented with data on the optical Balmer line emission and are used to study the geometrical distribution of the dust associated with the massive stars. We find that the reddening toward the starburst regions can be explained by the presence of foreground dust, either homogeneous or clumpy. The result suggests that there is little internal dust in the star-forming site. Mechanisms like shock waves and outflows produced by supernova explosions and hot star winds can be effective at destroying and removing the dust from inside the region.
id UFRGS-2_9aa983579968895e5b1138d88cc0b0c6
oai_identifier_str oai:www.lume.ufrgs.br:10183/108780
network_acronym_str UFRGS-2
network_name_str Repositório Institucional da UFRGS
repository_id_str
spelling Calzetti, DanielaKinney, Anne LouiseStorchi-Bergmann, Thaisa2015-01-07T02:10:57Z19960004-637Xhttp://hdl.handle.net/10183/108780000148838We present new observations of the near-infrared hydrogen recombination lines Paβ and Bry in the central starburst regions of 13 galaxies. The near-infrared data are supplemented with data on the optical Balmer line emission and are used to study the geometrical distribution of the dust associated with the massive stars. We find that the reddening toward the starburst regions can be explained by the presence of foreground dust, either homogeneous or clumpy. The result suggests that there is little internal dust in the star-forming site. Mechanisms like shock waves and outflows produced by supernova explosions and hot star winds can be effective at destroying and removing the dust from inside the region.application/pdfengThe astrophysical journal. Chicago. Vol. 458, no. 1, pt. 1 (Feb. 1996), p. 132-135Poeira cosmicaMateria interestelarEspectros infravermelhosEspectros astronômicosPoeira cosmicaGaláxias ativasDust, extinctionGalaxies: ISMGalaxies: starburstInfrared: galaxiesDust obscuration in starburst galaxies from near-infrared spectroscopyEstrangeiroinfo:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/openAccessreponame:Repositório Institucional da UFRGSinstname:Universidade Federal do Rio Grande do Sul (UFRGS)instacron:UFRGSORIGINAL000148838.pdf000148838.pdfTexto completo (inglês)application/pdf109400http://www.lume.ufrgs.br/bitstream/10183/108780/1/000148838.pdf155959a37c09d8e45eca2360c006b9eaMD51TEXT000148838.pdf.txt000148838.pdf.txtExtracted Texttext/plain88http://www.lume.ufrgs.br/bitstream/10183/108780/2/000148838.pdf.txt3573897b24dc3d0ae118f9246edd8e3aMD52THUMBNAIL000148838.pdf.jpg000148838.pdf.jpgGenerated Thumbnailimage/jpeg2149http://www.lume.ufrgs.br/bitstream/10183/108780/3/000148838.pdf.jpg1935d5309cc2e6b6233e771ecb6fd0abMD5310183/1087802018-10-23 08:34:40.239oai:www.lume.ufrgs.br:10183/108780Repositório de PublicaçõesPUBhttps://lume.ufrgs.br/oai/requestopendoar:2018-10-23T11:34:40Repositório Institucional da UFRGS - Universidade Federal do Rio Grande do Sul (UFRGS)false
dc.title.pt_BR.fl_str_mv Dust obscuration in starburst galaxies from near-infrared spectroscopy
title Dust obscuration in starburst galaxies from near-infrared spectroscopy
spellingShingle Dust obscuration in starburst galaxies from near-infrared spectroscopy
Calzetti, Daniela
Poeira cosmica
Materia interestelar
Espectros infravermelhos
Espectros astronômicos
Poeira cosmica
Galáxias ativas
Dust, extinction
Galaxies: ISM
Galaxies: starburst
Infrared: galaxies
title_short Dust obscuration in starburst galaxies from near-infrared spectroscopy
title_full Dust obscuration in starburst galaxies from near-infrared spectroscopy
title_fullStr Dust obscuration in starburst galaxies from near-infrared spectroscopy
title_full_unstemmed Dust obscuration in starburst galaxies from near-infrared spectroscopy
title_sort Dust obscuration in starburst galaxies from near-infrared spectroscopy
author Calzetti, Daniela
author_facet Calzetti, Daniela
Kinney, Anne Louise
Storchi-Bergmann, Thaisa
author_role author
author2 Kinney, Anne Louise
Storchi-Bergmann, Thaisa
author2_role author
author
dc.contributor.author.fl_str_mv Calzetti, Daniela
Kinney, Anne Louise
Storchi-Bergmann, Thaisa
dc.subject.por.fl_str_mv Poeira cosmica
Materia interestelar
Espectros infravermelhos
Espectros astronômicos
Poeira cosmica
Galáxias ativas
topic Poeira cosmica
Materia interestelar
Espectros infravermelhos
Espectros astronômicos
Poeira cosmica
Galáxias ativas
Dust, extinction
Galaxies: ISM
Galaxies: starburst
Infrared: galaxies
dc.subject.eng.fl_str_mv Dust, extinction
Galaxies: ISM
Galaxies: starburst
Infrared: galaxies
description We present new observations of the near-infrared hydrogen recombination lines Paβ and Bry in the central starburst regions of 13 galaxies. The near-infrared data are supplemented with data on the optical Balmer line emission and are used to study the geometrical distribution of the dust associated with the massive stars. We find that the reddening toward the starburst regions can be explained by the presence of foreground dust, either homogeneous or clumpy. The result suggests that there is little internal dust in the star-forming site. Mechanisms like shock waves and outflows produced by supernova explosions and hot star winds can be effective at destroying and removing the dust from inside the region.
publishDate 1996
dc.date.issued.fl_str_mv 1996
dc.date.accessioned.fl_str_mv 2015-01-07T02:10:57Z
dc.type.driver.fl_str_mv Estrangeiro
info:eu-repo/semantics/article
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
format article
status_str publishedVersion
dc.identifier.uri.fl_str_mv http://hdl.handle.net/10183/108780
dc.identifier.issn.pt_BR.fl_str_mv 0004-637X
dc.identifier.nrb.pt_BR.fl_str_mv 000148838
identifier_str_mv 0004-637X
000148838
url http://hdl.handle.net/10183/108780
dc.language.iso.fl_str_mv eng
language eng
dc.relation.ispartof.pt_BR.fl_str_mv The astrophysical journal. Chicago. Vol. 458, no. 1, pt. 1 (Feb. 1996), p. 132-135
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv application/pdf
dc.source.none.fl_str_mv reponame:Repositório Institucional da UFRGS
instname:Universidade Federal do Rio Grande do Sul (UFRGS)
instacron:UFRGS
instname_str Universidade Federal do Rio Grande do Sul (UFRGS)
instacron_str UFRGS
institution UFRGS
reponame_str Repositório Institucional da UFRGS
collection Repositório Institucional da UFRGS
bitstream.url.fl_str_mv http://www.lume.ufrgs.br/bitstream/10183/108780/1/000148838.pdf
http://www.lume.ufrgs.br/bitstream/10183/108780/2/000148838.pdf.txt
http://www.lume.ufrgs.br/bitstream/10183/108780/3/000148838.pdf.jpg
bitstream.checksum.fl_str_mv 155959a37c09d8e45eca2360c006b9ea
3573897b24dc3d0ae118f9246edd8e3a
1935d5309cc2e6b6233e771ecb6fd0ab
bitstream.checksumAlgorithm.fl_str_mv MD5
MD5
MD5
repository.name.fl_str_mv Repositório Institucional da UFRGS - Universidade Federal do Rio Grande do Sul (UFRGS)
repository.mail.fl_str_mv
_version_ 1801224861618536448

Registros relacionados