Chemo dynamics of Blue Compact Dwarf galaxies
- Autores
- Campuzano Castro, Federico; Hägele, Guillermo Federico; Bosch, Guillermo Luis; Firpo, Verónica; Morrell, Nidia Irene; Cardaci, Mónica Viviana
- Año de publicación
- 2016
- Idioma
- inglés
- Tipo de recurso
- documento de conferencia
- Estado
- versión publicada
- Descripción
- This work presents a brief summary of the analysis we are performing on the physical and chemical properties of the ionizing gas in star-forming regions belonging to two Blue Compact Dwarf galaxies (BCDs), using high resolution echelle spectra Our aim is to perform a detailed study of the Chemodynamics on BCDs. To do that, we use our own Python code using the LMF1T (Non-Linear Least-Squares Minimization and Curve-Fitting for Python) package. We deconvolve the emission-line profiles fitting several gaussians to the different kinematical components to be able to estimate the properties and. the nature of the ionized gas. Cur next step is to use the kinematical information to perform the chemical abundance analysis and to infer the physical properties of the gas (the chemodynamical study) by using the methodology published in Hagele et al. (2008, 2012).
Instituto de Astrofísica de La Plata - Materia
-
Ciencias Astronómicas
ionizing gas
star-forming regions
physical and chemical properties - 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:10915/165641
Ver los metadatos del registro completo
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Chemo dynamics of Blue Compact Dwarf galaxiesCampuzano Castro, FedericoHägele, Guillermo FedericoBosch, Guillermo LuisFirpo, VerónicaMorrell, Nidia IreneCardaci, Mónica VivianaCiencias Astronómicasionizing gasstar-forming regionsphysical and chemical propertiesThis work presents a brief summary of the analysis we are performing on the physical and chemical properties of the ionizing gas in star-forming regions belonging to two Blue Compact Dwarf galaxies (BCDs), using high resolution echelle spectra Our aim is to perform a detailed study of the Chemodynamics on BCDs. To do that, we use our own Python code using the LMF1T (Non-Linear Least-Squares Minimization and Curve-Fitting for Python) package. We deconvolve the emission-line profiles fitting several gaussians to the different kinematical components to be able to estimate the properties and. the nature of the ionized gas. Cur next step is to use the kinematical information to perform the chemical abundance analysis and to infer the physical properties of the gas (the chemodynamical study) by using the methodology published in Hagele et al. (2008, 2012).Instituto de Astrofísica de La Plata2016-11info:eu-repo/semantics/conferenceObjectinfo:eu-repo/semantics/publishedVersionObjeto de conferenciahttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdf189-193http://sedici.unlp.edu.ar/handle/10915/165641enginfo:eu-repo/semantics/altIdentifier/isbn/978-987-24948-5-8info: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:UNLP2025-09-29T11:43:56Zoai:sedici.unlp.edu.ar:10915/165641Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:43:57.097SEDICI (UNLP) - Universidad Nacional de La Platafalse |
dc.title.none.fl_str_mv |
Chemo dynamics of Blue Compact Dwarf galaxies |
title |
Chemo dynamics of Blue Compact Dwarf galaxies |
spellingShingle |
Chemo dynamics of Blue Compact Dwarf galaxies Campuzano Castro, Federico Ciencias Astronómicas ionizing gas star-forming regions physical and chemical properties |
title_short |
Chemo dynamics of Blue Compact Dwarf galaxies |
title_full |
Chemo dynamics of Blue Compact Dwarf galaxies |
title_fullStr |
Chemo dynamics of Blue Compact Dwarf galaxies |
title_full_unstemmed |
Chemo dynamics of Blue Compact Dwarf galaxies |
title_sort |
Chemo dynamics of Blue Compact Dwarf galaxies |
dc.creator.none.fl_str_mv |
Campuzano Castro, Federico Hägele, Guillermo Federico Bosch, Guillermo Luis Firpo, Verónica Morrell, Nidia Irene Cardaci, Mónica Viviana |
author |
Campuzano Castro, Federico |
author_facet |
Campuzano Castro, Federico Hägele, Guillermo Federico Bosch, Guillermo Luis Firpo, Verónica Morrell, Nidia Irene Cardaci, Mónica Viviana |
author_role |
author |
author2 |
Hägele, Guillermo Federico Bosch, Guillermo Luis Firpo, Verónica Morrell, Nidia Irene Cardaci, Mónica Viviana |
author2_role |
author author author author author |
dc.subject.none.fl_str_mv |
Ciencias Astronómicas ionizing gas star-forming regions physical and chemical properties |
topic |
Ciencias Astronómicas ionizing gas star-forming regions physical and chemical properties |
dc.description.none.fl_txt_mv |
This work presents a brief summary of the analysis we are performing on the physical and chemical properties of the ionizing gas in star-forming regions belonging to two Blue Compact Dwarf galaxies (BCDs), using high resolution echelle spectra Our aim is to perform a detailed study of the Chemodynamics on BCDs. To do that, we use our own Python code using the LMF1T (Non-Linear Least-Squares Minimization and Curve-Fitting for Python) package. We deconvolve the emission-line profiles fitting several gaussians to the different kinematical components to be able to estimate the properties and. the nature of the ionized gas. Cur next step is to use the kinematical information to perform the chemical abundance analysis and to infer the physical properties of the gas (the chemodynamical study) by using the methodology published in Hagele et al. (2008, 2012). Instituto de Astrofísica de La Plata |
description |
This work presents a brief summary of the analysis we are performing on the physical and chemical properties of the ionizing gas in star-forming regions belonging to two Blue Compact Dwarf galaxies (BCDs), using high resolution echelle spectra Our aim is to perform a detailed study of the Chemodynamics on BCDs. To do that, we use our own Python code using the LMF1T (Non-Linear Least-Squares Minimization and Curve-Fitting for Python) package. We deconvolve the emission-line profiles fitting several gaussians to the different kinematical components to be able to estimate the properties and. the nature of the ionized gas. Cur next step is to use the kinematical information to perform the chemical abundance analysis and to infer the physical properties of the gas (the chemodynamical study) by using the methodology published in Hagele et al. (2008, 2012). |
publishDate |
2016 |
dc.date.none.fl_str_mv |
2016-11 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/conferenceObject info:eu-repo/semantics/publishedVersion Objeto de conferencia http://purl.org/coar/resource_type/c_5794 info:ar-repo/semantics/documentoDeConferencia |
format |
conferenceObject |
status_str |
publishedVersion |
dc.identifier.none.fl_str_mv |
http://sedici.unlp.edu.ar/handle/10915/165641 |
url |
http://sedici.unlp.edu.ar/handle/10915/165641 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/isbn/978-987-24948-5-8 |
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) |
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openAccess |
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http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
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application/pdf 189-193 |
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SEDICI (UNLP) - Universidad Nacional de La Plata |
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