Studying the kinematics of the giant star-forming region 30 Doradus . I.The data

Autores
Torres-Flores, S.; Barbá, Rodolfo; Maíz Apellániz, Jesús; Rubio, Mónica; Bosch, Guillermo Luis; Henault-Brunet, V.; Evans, Chris J.
Año de publicación
2013
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We present high-quality VLT-FLAMES optical spectroscopy of the nebular gas in the giant star-forming region 30 Doradus. In this paper, the first of a series, we introduce our observations and discuss the main kinematic features of 30 Dor, as revealed by the spectroscopy of the ionized gas in the region. The primary data set consists of regular grid of nebular observations, which we used to produce a spectroscopic datacube of 30 Dor, centered on the massive star cluster R136 and covering a field-of-view of 10´ × 10´. The main emission lines present in the datacube are from Hα and [Nii] λλ6548, 6584. The Hα emission-line profile varies across the region from simple single-peaked emission to complex, multiple-component profiles, suggesting that different physical mechanisms are acting on the excited gas. To analyse the gas kinematics we fit Gaussian profiles to the observed Hα features. Unexpectedly, the narrowest Hα profile in our sample lies close to the supernova remnant 30 Dor B. We present maps of the velocity field and velocity dispersion across 30 Dor, finding five previously unclassified expanding structures. These maps highlight the kinematic richness of 30 Dor (e.g. supersonic motions), which will be analysed in future papers.
Fil: Torres-Flores, S.. Departamento de Física. Universidad de La Serena; Chile;
Fil: Barbá, Rodolfo. Instituto de Ciencias Astronómicas de la Tierra y del Espacio; Argentina;
Fil: Maíz Apellániz, Jesús. Instituto de Astrofísica de Andalucía-CSIC; España;
Fil: Rubio, Mónica. Departamento de Astronomía, Universidad de Chile; Chile;
Fil: Bosch, Guillermo Luis. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina;
Fil: Henault-Brunet, V.. Institute for Astronomy. Royal Observatory Edinburgh; Argentina;
Fil: Evans, Chris J.. UK Astronomy Technology Centre. Royal Observatory Edinburgh; Reino Unido;
Materia
ISM: bubbles
ISM: kinematics and dynamics
HII regions
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/631
Acceder
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oai_identifier_str oai:ri.conicet.gov.ar:11336/631
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Studying the kinematics of the giant star-forming region 30 Doradus . I.The dataTorres-Flores, S.Barbá, RodolfoMaíz Apellániz, JesúsRubio, MónicaBosch, Guillermo LuisHenault-Brunet, V.Evans, Chris J.ISM: bubblesISM: kinematics and dynamicsHII regionshttps://purl.org/becyt/ford/1https://purl.org/becyt/ford/1.3We present high-quality VLT-FLAMES optical spectroscopy of the nebular gas in the giant star-forming region 30 Doradus. In this paper, the first of a series, we introduce our observations and discuss the main kinematic features of 30 Dor, as revealed by the spectroscopy of the ionized gas in the region. The primary data set consists of regular grid of nebular observations, which we used to produce a spectroscopic datacube of 30 Dor, centered on the massive star cluster R136 and covering a field-of-view of 10´ × 10´. The main emission lines present in the datacube are from Hα and [Nii] λλ6548, 6584. The Hα emission-line profile varies across the region from simple single-peaked emission to complex, multiple-component profiles, suggesting that different physical mechanisms are acting on the excited gas. To analyse the gas kinematics we fit Gaussian profiles to the observed Hα features. Unexpectedly, the narrowest Hα profile in our sample lies close to the supernova remnant 30 Dor B. We present maps of the velocity field and velocity dispersion across 30 Dor, finding five previously unclassified expanding structures. These maps highlight the kinematic richness of 30 Dor (e.g. supersonic motions), which will be analysed in future papers.Fil: Torres-Flores, S.. Departamento de Física. Universidad de La Serena; Chile;Fil: Barbá, Rodolfo. Instituto de Ciencias Astronómicas de la Tierra y del Espacio; Argentina;Fil: Maíz Apellániz, Jesús. Instituto de Astrofísica de Andalucía-CSIC; España;Fil: Rubio, Mónica. Departamento de Astronomía, Universidad de Chile; Chile;Fil: Bosch, Guillermo Luis. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina;Fil: Henault-Brunet, V.. Institute for Astronomy. Royal Observatory Edinburgh; Argentina;Fil: Evans, Chris J.. UK Astronomy Technology Centre. Royal Observatory Edinburgh; Reino Unido;Edp Sciences S A2013-04-30info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/631Torres-Flores, S.; Barbá, Rodolfo; Maíz Apellániz, Jesús; Rubio, Mónica; Bosch, Guillermo Luis; Henault-Brunet, V.; Evans, Chris J.; Studying the kinematics of the giant star-forming region 30 Doradus . I.The data; Edp Sciences S A; Astronomy And Astrophysics; 555; 30-4-2013; 60-81;0004-6361enginfo:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201220474info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:18:35Zoai:ri.conicet.gov.ar:11336/631instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 10:18:35.349CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Studying the kinematics of the giant star-forming region 30 Doradus . I.The data
title Studying the kinematics of the giant star-forming region 30 Doradus . I.The data
spellingShingle Studying the kinematics of the giant star-forming region 30 Doradus . I.The data
Torres-Flores, S.
ISM: bubbles
ISM: kinematics and dynamics
HII regions
title_short Studying the kinematics of the giant star-forming region 30 Doradus . I.The data
title_full Studying the kinematics of the giant star-forming region 30 Doradus . I.The data
title_fullStr Studying the kinematics of the giant star-forming region 30 Doradus . I.The data
title_full_unstemmed Studying the kinematics of the giant star-forming region 30 Doradus . I.The data
title_sort Studying the kinematics of the giant star-forming region 30 Doradus . I.The data
dc.creator.none.fl_str_mv Torres-Flores, S.
Barbá, Rodolfo
Maíz Apellániz, Jesús
Rubio, Mónica
Bosch, Guillermo Luis
Henault-Brunet, V.
Evans, Chris J.
author Torres-Flores, S.
author_facet Torres-Flores, S.
Barbá, Rodolfo
Maíz Apellániz, Jesús
Rubio, Mónica
Bosch, Guillermo Luis
Henault-Brunet, V.
Evans, Chris J.
author_role author
author2 Barbá, Rodolfo
Maíz Apellániz, Jesús
Rubio, Mónica
Bosch, Guillermo Luis
Henault-Brunet, V.
Evans, Chris J.
author2_role author
author
author
author
author
author
dc.subject.none.fl_str_mv ISM: bubbles
ISM: kinematics and dynamics
HII regions
topic ISM: bubbles
ISM: kinematics and dynamics
HII regions
purl_subject.fl_str_mv https://purl.org/becyt/ford/1
https://purl.org/becyt/ford/1.3
dc.description.none.fl_txt_mv We present high-quality VLT-FLAMES optical spectroscopy of the nebular gas in the giant star-forming region 30 Doradus. In this paper, the first of a series, we introduce our observations and discuss the main kinematic features of 30 Dor, as revealed by the spectroscopy of the ionized gas in the region. The primary data set consists of regular grid of nebular observations, which we used to produce a spectroscopic datacube of 30 Dor, centered on the massive star cluster R136 and covering a field-of-view of 10´ × 10´. The main emission lines present in the datacube are from Hα and [Nii] λλ6548, 6584. The Hα emission-line profile varies across the region from simple single-peaked emission to complex, multiple-component profiles, suggesting that different physical mechanisms are acting on the excited gas. To analyse the gas kinematics we fit Gaussian profiles to the observed Hα features. Unexpectedly, the narrowest Hα profile in our sample lies close to the supernova remnant 30 Dor B. We present maps of the velocity field and velocity dispersion across 30 Dor, finding five previously unclassified expanding structures. These maps highlight the kinematic richness of 30 Dor (e.g. supersonic motions), which will be analysed in future papers.
Fil: Torres-Flores, S.. Departamento de Física. Universidad de La Serena; Chile;
Fil: Barbá, Rodolfo. Instituto de Ciencias Astronómicas de la Tierra y del Espacio; Argentina;
Fil: Maíz Apellániz, Jesús. Instituto de Astrofísica de Andalucía-CSIC; España;
Fil: Rubio, Mónica. Departamento de Astronomía, Universidad de Chile; Chile;
Fil: Bosch, Guillermo Luis. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina;
Fil: Henault-Brunet, V.. Institute for Astronomy. Royal Observatory Edinburgh; Argentina;
Fil: Evans, Chris J.. UK Astronomy Technology Centre. Royal Observatory Edinburgh; Reino Unido;
description We present high-quality VLT-FLAMES optical spectroscopy of the nebular gas in the giant star-forming region 30 Doradus. In this paper, the first of a series, we introduce our observations and discuss the main kinematic features of 30 Dor, as revealed by the spectroscopy of the ionized gas in the region. The primary data set consists of regular grid of nebular observations, which we used to produce a spectroscopic datacube of 30 Dor, centered on the massive star cluster R136 and covering a field-of-view of 10´ × 10´. The main emission lines present in the datacube are from Hα and [Nii] λλ6548, 6584. The Hα emission-line profile varies across the region from simple single-peaked emission to complex, multiple-component profiles, suggesting that different physical mechanisms are acting on the excited gas. To analyse the gas kinematics we fit Gaussian profiles to the observed Hα features. Unexpectedly, the narrowest Hα profile in our sample lies close to the supernova remnant 30 Dor B. We present maps of the velocity field and velocity dispersion across 30 Dor, finding five previously unclassified expanding structures. These maps highlight the kinematic richness of 30 Dor (e.g. supersonic motions), which will be analysed in future papers.
publishDate 2013
dc.date.none.fl_str_mv 2013-04-30
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/631
Torres-Flores, S.; Barbá, Rodolfo; Maíz Apellániz, Jesús; Rubio, Mónica; Bosch, Guillermo Luis; Henault-Brunet, V.; Evans, Chris J.; Studying the kinematics of the giant star-forming region 30 Doradus . I.The data; Edp Sciences S A; Astronomy And Astrophysics; 555; 30-4-2013; 60-81;
0004-6361
url http://hdl.handle.net/11336/631
identifier_str_mv Torres-Flores, S.; Barbá, Rodolfo; Maíz Apellániz, Jesús; Rubio, Mónica; Bosch, Guillermo Luis; Henault-Brunet, V.; Evans, Chris J.; Studying the kinematics of the giant star-forming region 30 Doradus . I.The data; Edp Sciences S A; Astronomy And Astrophysics; 555; 30-4-2013; 60-81;
0004-6361
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201220474
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv Edp Sciences S A
publisher.none.fl_str_mv Edp Sciences S A
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
_version_ 1844614149543297024
score 13.070432

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