Integral field spectroscopy of HII region complexes: the outer disc of NGC6946
- Autores
- García Benito, Rubén; Díaz, A.; Hägele, Guillermo Federico; Pérez Montero, E.; López, Jesús; Vílchez, J. M.; Pérez, Enrique; Terlevich, Elena; Terlevich, Roberto; Rosa González, Daniel
- Año de publicación
- 2010
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Integral field spectroscopy obtained with the Potsdam Multi-Aperture Spectrophotometer Fiber Package (PPak) and the 3.5-m telescope at the Calar Alto Observatory has been used to study an outer H II region complex in the well-studied galaxy NGC 6946. This technique provides detailed maps of the region in different emission lines, yielding spatially resolved information about the physical properties of the gas. The configuration was chosen to cover the whole spectrum from 3600 up to 10 000 Å, allowing the measurement of the near-infrared [S III] lines. We selected four luminous knots to perform a detailed integrated spectroscopic analysis of these structures and of the whole PPak field of view (FOV). For all the knots the electron density has been found to be very similar and below 100 cm−3. The [O III] electron temperature was measured in knots A, B, C and in the integrated PPak field, and was found to be around 8000 K. The temperatures of [O II] and [S III] were estimated in the four cases. The elemental abundances computed from the ‘direct method’ are typical of high-metallicity disc H II regions, with a mean value of 12+log(O/H) = 8.65, comparable to what has been found in this galaxy by other authors for regions at similar galactocentric distance. Therefore a remarkable abundance uniformity is found despite the different excitations found throughout the nebula. However, due to the quality of the data, the electron temperatures and metallicities obtained have associated errors comparable to the typical dispersion found in empirical calibrations.
Fil: García Benito, Rubén. Peking University. Kavli Institute of Astronomy and Astrophysics; China
Fil: Díaz, A.. Universidad Autónoma de Madrid. Departamento de Física Teorica; España
Fil: Hägele, Guillermo Federico. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto de Astrofísica de La Plata; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: Pérez Montero, E.. Consejo Superior de Investigaciones Cientificas. Instituto de Astrofísica de Andalucía; España
Fil: López, Jesús . INAOE; México
Fil: Vílchez, J. M.. Consejo Superior de Investigaciones Cientificas. Instituto de Astrofísica de Andalucía; España
Fil: Pérez, Enrique. Consejo Superior de Investigaciones Cientificas. Instituto de Astrofísica de Andalucía; España
Fil: Terlevich, Elena . INAOE; México
Fil: Terlevich, Roberto . INAOE; México
Fil: Rosa González, Daniel. INAOE; México - Materia
-
Abundances (ISM)
HII regions
Interstellar medium
Spectroscopic techniques - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/9845
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Integral field spectroscopy of HII region complexes: the outer disc of NGC6946García Benito, RubénDíaz, A.Hägele, Guillermo FedericoPérez Montero, E.López, Jesús Vílchez, J. M.Pérez, EnriqueTerlevich, Elena Terlevich, Roberto Rosa González, DanielAbundances (ISM)HII regionsInterstellar mediumSpectroscopic techniqueshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Integral field spectroscopy obtained with the Potsdam Multi-Aperture Spectrophotometer Fiber Package (PPak) and the 3.5-m telescope at the Calar Alto Observatory has been used to study an outer H II region complex in the well-studied galaxy NGC 6946. This technique provides detailed maps of the region in different emission lines, yielding spatially resolved information about the physical properties of the gas. The configuration was chosen to cover the whole spectrum from 3600 up to 10 000 Å, allowing the measurement of the near-infrared [S III] lines. We selected four luminous knots to perform a detailed integrated spectroscopic analysis of these structures and of the whole PPak field of view (FOV). For all the knots the electron density has been found to be very similar and below 100 cm−3. The [O III] electron temperature was measured in knots A, B, C and in the integrated PPak field, and was found to be around 8000 K. The temperatures of [O II] and [S III] were estimated in the four cases. The elemental abundances computed from the ‘direct method’ are typical of high-metallicity disc H II regions, with a mean value of 12+log(O/H) = 8.65, comparable to what has been found in this galaxy by other authors for regions at similar galactocentric distance. Therefore a remarkable abundance uniformity is found despite the different excitations found throughout the nebula. However, due to the quality of the data, the electron temperatures and metallicities obtained have associated errors comparable to the typical dispersion found in empirical calibrations.Fil: García Benito, Rubén. Peking University. Kavli Institute of Astronomy and Astrophysics; ChinaFil: Díaz, A.. Universidad Autónoma de Madrid. Departamento de Física Teorica; EspañaFil: Hägele, Guillermo Federico. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto de Astrofísica de La Plata; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; ArgentinaFil: Pérez Montero, E.. Consejo Superior de Investigaciones Cientificas. Instituto de Astrofísica de Andalucía; EspañaFil: López, Jesús . INAOE; MéxicoFil: Vílchez, J. M.. Consejo Superior de Investigaciones Cientificas. Instituto de Astrofísica de Andalucía; EspañaFil: Pérez, Enrique. Consejo Superior de Investigaciones Cientificas. Instituto de Astrofísica de Andalucía; EspañaFil: Terlevich, Elena . INAOE; MéxicoFil: Terlevich, Roberto . INAOE; MéxicoFil: Rosa González, Daniel. INAOE; MéxicoOxford University Press2010-11info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/9845García Benito, Rubén; Díaz, A.; Hägele, Guillermo Federico; Pérez Montero, E.; López, Jesús ; et al.; Integral field spectroscopy of HII region complexes: the outer disc of NGC6946; Oxford University Press; Monthly Notices Of The Royal Astronomical Society; 408; 4; 11-2010; 2234-22550035-8711enginfo:eu-repo/semantics/altIdentifier/url/http://mnras.oxfordjournals.org/content/408/4/2234info:eu-repo/semantics/altIdentifier/doi/10.1111/j.1365-2966.2010.17269.xinfo:eu-repo/semantics/altIdentifier/url/http://onlinelibrary.wiley.com/doi/10.1111/j.1365-2966.2010.17269.x/fullinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:32:37Zoai:ri.conicet.gov.ar:11336/9845instacron: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 09:32:37.543CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Integral field spectroscopy of HII region complexes: the outer disc of NGC6946 |
title |
Integral field spectroscopy of HII region complexes: the outer disc of NGC6946 |
spellingShingle |
Integral field spectroscopy of HII region complexes: the outer disc of NGC6946 García Benito, Rubén Abundances (ISM) HII regions Interstellar medium Spectroscopic techniques |
title_short |
Integral field spectroscopy of HII region complexes: the outer disc of NGC6946 |
title_full |
Integral field spectroscopy of HII region complexes: the outer disc of NGC6946 |
title_fullStr |
Integral field spectroscopy of HII region complexes: the outer disc of NGC6946 |
title_full_unstemmed |
Integral field spectroscopy of HII region complexes: the outer disc of NGC6946 |
title_sort |
Integral field spectroscopy of HII region complexes: the outer disc of NGC6946 |
dc.creator.none.fl_str_mv |
García Benito, Rubén Díaz, A. Hägele, Guillermo Federico Pérez Montero, E. López, Jesús Vílchez, J. M. Pérez, Enrique Terlevich, Elena Terlevich, Roberto Rosa González, Daniel |
author |
García Benito, Rubén |
author_facet |
García Benito, Rubén Díaz, A. Hägele, Guillermo Federico Pérez Montero, E. López, Jesús Vílchez, J. M. Pérez, Enrique Terlevich, Elena Terlevich, Roberto Rosa González, Daniel |
author_role |
author |
author2 |
Díaz, A. Hägele, Guillermo Federico Pérez Montero, E. López, Jesús Vílchez, J. M. Pérez, Enrique Terlevich, Elena Terlevich, Roberto Rosa González, Daniel |
author2_role |
author author author author author author author author author |
dc.subject.none.fl_str_mv |
Abundances (ISM) HII regions Interstellar medium Spectroscopic techniques |
topic |
Abundances (ISM) HII regions Interstellar medium Spectroscopic techniques |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
Integral field spectroscopy obtained with the Potsdam Multi-Aperture Spectrophotometer Fiber Package (PPak) and the 3.5-m telescope at the Calar Alto Observatory has been used to study an outer H II region complex in the well-studied galaxy NGC 6946. This technique provides detailed maps of the region in different emission lines, yielding spatially resolved information about the physical properties of the gas. The configuration was chosen to cover the whole spectrum from 3600 up to 10 000 Å, allowing the measurement of the near-infrared [S III] lines. We selected four luminous knots to perform a detailed integrated spectroscopic analysis of these structures and of the whole PPak field of view (FOV). For all the knots the electron density has been found to be very similar and below 100 cm−3. The [O III] electron temperature was measured in knots A, B, C and in the integrated PPak field, and was found to be around 8000 K. The temperatures of [O II] and [S III] were estimated in the four cases. The elemental abundances computed from the ‘direct method’ are typical of high-metallicity disc H II regions, with a mean value of 12+log(O/H) = 8.65, comparable to what has been found in this galaxy by other authors for regions at similar galactocentric distance. Therefore a remarkable abundance uniformity is found despite the different excitations found throughout the nebula. However, due to the quality of the data, the electron temperatures and metallicities obtained have associated errors comparable to the typical dispersion found in empirical calibrations. Fil: García Benito, Rubén. Peking University. Kavli Institute of Astronomy and Astrophysics; China Fil: Díaz, A.. Universidad Autónoma de Madrid. Departamento de Física Teorica; España Fil: Hägele, Guillermo Federico. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto de Astrofísica de La Plata; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina Fil: Pérez Montero, E.. Consejo Superior de Investigaciones Cientificas. Instituto de Astrofísica de Andalucía; España Fil: López, Jesús . INAOE; México Fil: Vílchez, J. M.. Consejo Superior de Investigaciones Cientificas. Instituto de Astrofísica de Andalucía; España Fil: Pérez, Enrique. Consejo Superior de Investigaciones Cientificas. Instituto de Astrofísica de Andalucía; España Fil: Terlevich, Elena . INAOE; México Fil: Terlevich, Roberto . INAOE; México Fil: Rosa González, Daniel. INAOE; México |
description |
Integral field spectroscopy obtained with the Potsdam Multi-Aperture Spectrophotometer Fiber Package (PPak) and the 3.5-m telescope at the Calar Alto Observatory has been used to study an outer H II region complex in the well-studied galaxy NGC 6946. This technique provides detailed maps of the region in different emission lines, yielding spatially resolved information about the physical properties of the gas. The configuration was chosen to cover the whole spectrum from 3600 up to 10 000 Å, allowing the measurement of the near-infrared [S III] lines. We selected four luminous knots to perform a detailed integrated spectroscopic analysis of these structures and of the whole PPak field of view (FOV). For all the knots the electron density has been found to be very similar and below 100 cm−3. The [O III] electron temperature was measured in knots A, B, C and in the integrated PPak field, and was found to be around 8000 K. The temperatures of [O II] and [S III] were estimated in the four cases. The elemental abundances computed from the ‘direct method’ are typical of high-metallicity disc H II regions, with a mean value of 12+log(O/H) = 8.65, comparable to what has been found in this galaxy by other authors for regions at similar galactocentric distance. Therefore a remarkable abundance uniformity is found despite the different excitations found throughout the nebula. However, due to the quality of the data, the electron temperatures and metallicities obtained have associated errors comparable to the typical dispersion found in empirical calibrations. |
publishDate |
2010 |
dc.date.none.fl_str_mv |
2010-11 |
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/11336/9845 García Benito, Rubén; Díaz, A.; Hägele, Guillermo Federico; Pérez Montero, E.; López, Jesús ; et al.; Integral field spectroscopy of HII region complexes: the outer disc of NGC6946; Oxford University Press; Monthly Notices Of The Royal Astronomical Society; 408; 4; 11-2010; 2234-2255 0035-8711 |
url |
http://hdl.handle.net/11336/9845 |
identifier_str_mv |
García Benito, Rubén; Díaz, A.; Hägele, Guillermo Federico; Pérez Montero, E.; López, Jesús ; et al.; Integral field spectroscopy of HII region complexes: the outer disc of NGC6946; Oxford University Press; Monthly Notices Of The Royal Astronomical Society; 408; 4; 11-2010; 2234-2255 0035-8711 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/url/http://mnras.oxfordjournals.org/content/408/4/2234 info:eu-repo/semantics/altIdentifier/doi/10.1111/j.1365-2966.2010.17269.x info:eu-repo/semantics/altIdentifier/url/http://onlinelibrary.wiley.com/doi/10.1111/j.1365-2966.2010.17269.x/full |
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 |
Oxford University Press |
publisher.none.fl_str_mv |
Oxford University Press |
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 |
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1844612996546953216 |
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13.070432 |