High-resolution spectroscopy of the blue compact dwarf galaxy Haro 15 – II. Chemodynamics
- Autores
- Hägele, Guillermo Federico; Firpo, Verónica; Bosch, Guillermo Luis; Díaz, Angeles I.; Morrell, Nidia Irene
- Año de publicación
- 2012
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We present a detailed study of the physical properties of the nebular material in four starforming knots of the blue compact dwarf galaxy Haro 15. Using long-slit and echelle spectroscopy obtained at Las Campanas Observatory, we study the physical conditions (electron density and temperatures), ionic and total chemical abundances of several atoms, reddening and ionization structure, for the global flux and for the different kinematical components. The latter was derived by comparing the oxygen and sulphur ionic ratios to their corresponding observed emission-line ratios (the η and η 'plots) in different regions of the galaxy. Applying the direct method or empirical relationships for abundance determination, we perform a comparative analysis between these regions. The similarities found in the ionization structure of the different kinematical components imply that the effective temperatures of the ionizing radiation fields are very similar in spite of some small differences in the ionization state of the different elements. Therefore, the different gaseous kinematical components identified in each star-forming knot are probably ionized by the same star cluster. However, the difference in the ionizing structure of the two knots with knot A showing a lower effective temperature than knot B suggests a different evolutionary stage for them consistent with the presence of an older and more evolved stellar population in the first.
Instituto de Astrofísica de La Plata - Materia
-
Ciencias Astronómicas
ISM: abundances
H II regions
Galaxies: abundances
Galaxies: fundamental parameters
Galaxies: individual: Haro 15
Galaxies: starburst - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/126095
Ver los metadatos del registro completo
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High-resolution spectroscopy of the blue compact dwarf galaxy Haro 15 – II. ChemodynamicsHägele, Guillermo FedericoFirpo, VerónicaBosch, Guillermo LuisDíaz, Angeles I.Morrell, Nidia IreneCiencias AstronómicasISM: abundancesH II regionsGalaxies: abundancesGalaxies: fundamental parametersGalaxies: individual: Haro 15Galaxies: starburstWe present a detailed study of the physical properties of the nebular material in four starforming knots of the blue compact dwarf galaxy Haro 15. Using long-slit and echelle spectroscopy obtained at Las Campanas Observatory, we study the physical conditions (electron density and temperatures), ionic and total chemical abundances of several atoms, reddening and ionization structure, for the global flux and for the different kinematical components. The latter was derived by comparing the oxygen and sulphur ionic ratios to their corresponding observed emission-line ratios (the η and η 'plots) in different regions of the galaxy. Applying the direct method or empirical relationships for abundance determination, we perform a comparative analysis between these regions. The similarities found in the ionization structure of the different kinematical components imply that the effective temperatures of the ionizing radiation fields are very similar in spite of some small differences in the ionization state of the different elements. Therefore, the different gaseous kinematical components identified in each star-forming knot are probably ionized by the same star cluster. However, the difference in the ionizing structure of the two knots with knot A showing a lower effective temperature than knot B suggests a different evolutionary stage for them consistent with the presence of an older and more evolved stellar population in the first.Instituto de Astrofísica de La Plata2012-04-10info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf3475-3494http://sedici.unlp.edu.ar/handle/10915/126095enginfo:eu-repo/semantics/altIdentifier/issn/0035-8711info:eu-repo/semantics/altIdentifier/issn/1365-2966info:eu-repo/semantics/altIdentifier/doi/10.1111/j.1365-2966.2012.20858.xinfo:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-09-29T11:30:14Zoai:sedici.unlp.edu.ar:10915/126095Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:30:14.339SEDICI (UNLP) - Universidad Nacional de La Platafalse |
dc.title.none.fl_str_mv |
High-resolution spectroscopy of the blue compact dwarf galaxy Haro 15 – II. Chemodynamics |
title |
High-resolution spectroscopy of the blue compact dwarf galaxy Haro 15 – II. Chemodynamics |
spellingShingle |
High-resolution spectroscopy of the blue compact dwarf galaxy Haro 15 – II. Chemodynamics Hägele, Guillermo Federico Ciencias Astronómicas ISM: abundances H II regions Galaxies: abundances Galaxies: fundamental parameters Galaxies: individual: Haro 15 Galaxies: starburst |
title_short |
High-resolution spectroscopy of the blue compact dwarf galaxy Haro 15 – II. Chemodynamics |
title_full |
High-resolution spectroscopy of the blue compact dwarf galaxy Haro 15 – II. Chemodynamics |
title_fullStr |
High-resolution spectroscopy of the blue compact dwarf galaxy Haro 15 – II. Chemodynamics |
title_full_unstemmed |
High-resolution spectroscopy of the blue compact dwarf galaxy Haro 15 – II. Chemodynamics |
title_sort |
High-resolution spectroscopy of the blue compact dwarf galaxy Haro 15 – II. Chemodynamics |
dc.creator.none.fl_str_mv |
Hägele, Guillermo Federico Firpo, Verónica Bosch, Guillermo Luis Díaz, Angeles I. Morrell, Nidia Irene |
author |
Hägele, Guillermo Federico |
author_facet |
Hägele, Guillermo Federico Firpo, Verónica Bosch, Guillermo Luis Díaz, Angeles I. Morrell, Nidia Irene |
author_role |
author |
author2 |
Firpo, Verónica Bosch, Guillermo Luis Díaz, Angeles I. Morrell, Nidia Irene |
author2_role |
author author author author |
dc.subject.none.fl_str_mv |
Ciencias Astronómicas ISM: abundances H II regions Galaxies: abundances Galaxies: fundamental parameters Galaxies: individual: Haro 15 Galaxies: starburst |
topic |
Ciencias Astronómicas ISM: abundances H II regions Galaxies: abundances Galaxies: fundamental parameters Galaxies: individual: Haro 15 Galaxies: starburst |
dc.description.none.fl_txt_mv |
We present a detailed study of the physical properties of the nebular material in four starforming knots of the blue compact dwarf galaxy Haro 15. Using long-slit and echelle spectroscopy obtained at Las Campanas Observatory, we study the physical conditions (electron density and temperatures), ionic and total chemical abundances of several atoms, reddening and ionization structure, for the global flux and for the different kinematical components. The latter was derived by comparing the oxygen and sulphur ionic ratios to their corresponding observed emission-line ratios (the η and η 'plots) in different regions of the galaxy. Applying the direct method or empirical relationships for abundance determination, we perform a comparative analysis between these regions. The similarities found in the ionization structure of the different kinematical components imply that the effective temperatures of the ionizing radiation fields are very similar in spite of some small differences in the ionization state of the different elements. Therefore, the different gaseous kinematical components identified in each star-forming knot are probably ionized by the same star cluster. However, the difference in the ionizing structure of the two knots with knot A showing a lower effective temperature than knot B suggests a different evolutionary stage for them consistent with the presence of an older and more evolved stellar population in the first. Instituto de Astrofísica de La Plata |
description |
We present a detailed study of the physical properties of the nebular material in four starforming knots of the blue compact dwarf galaxy Haro 15. Using long-slit and echelle spectroscopy obtained at Las Campanas Observatory, we study the physical conditions (electron density and temperatures), ionic and total chemical abundances of several atoms, reddening and ionization structure, for the global flux and for the different kinematical components. The latter was derived by comparing the oxygen and sulphur ionic ratios to their corresponding observed emission-line ratios (the η and η 'plots) in different regions of the galaxy. Applying the direct method or empirical relationships for abundance determination, we perform a comparative analysis between these regions. The similarities found in the ionization structure of the different kinematical components imply that the effective temperatures of the ionizing radiation fields are very similar in spite of some small differences in the ionization state of the different elements. Therefore, the different gaseous kinematical components identified in each star-forming knot are probably ionized by the same star cluster. However, the difference in the ionizing structure of the two knots with knot A showing a lower effective temperature than knot B suggests a different evolutionary stage for them consistent with the presence of an older and more evolved stellar population in the first. |
publishDate |
2012 |
dc.date.none.fl_str_mv |
2012-04-10 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion Articulo 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://sedici.unlp.edu.ar/handle/10915/126095 |
url |
http://sedici.unlp.edu.ar/handle/10915/126095 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/issn/0035-8711 info:eu-repo/semantics/altIdentifier/issn/1365-2966 info:eu-repo/semantics/altIdentifier/doi/10.1111/j.1365-2966.2012.20858.x |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
dc.format.none.fl_str_mv |
application/pdf 3475-3494 |
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SEDICI (UNLP) - Universidad Nacional de La Plata |
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