Chemodynamics 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 LMFIT (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. Our 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 Hägele et al. (2008, 2012).
Instituto de Astrofísica de La Plata - Materia
-
Ciencias Astronómicas
ionizing gas
physical and chemical properties
Blue Compact Dwarf galaxies - 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:10915/165265
Ver los metadatos del registro completo
id |
SEDICI_493dcb7fe536f05f4e81e2c9aabb8c95 |
---|---|
oai_identifier_str |
oai:sedici.unlp.edu.ar:10915/165265 |
network_acronym_str |
SEDICI |
repository_id_str |
1329 |
network_name_str |
SEDICI (UNLP) |
spelling |
Chemodynamics of blue compact dwarf galaxiesCampuzano Castro, FedericoHägele, Guillermo FedericoBosch, Guillermo LuisFirpo, VerónicaMorrell, Nidia IreneCardaci, Mónica VivianaCiencias Astronómicasionizing gasphysical and chemical propertiesBlue Compact Dwarf galaxiesThis 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 LMFIT (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. Our 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 Hägele 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/10915/165265enginfo: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:UNLP2025-09-29T11:43:50Zoai:sedici.unlp.edu.ar:10915/165265Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:43:50.912SEDICI (UNLP) - Universidad Nacional de La Platafalse |
dc.title.none.fl_str_mv |
Chemodynamics of blue compact dwarf galaxies |
title |
Chemodynamics of blue compact dwarf galaxies |
spellingShingle |
Chemodynamics of blue compact dwarf galaxies Campuzano Castro, Federico Ciencias Astronómicas ionizing gas physical and chemical properties Blue Compact Dwarf galaxies |
title_short |
Chemodynamics of blue compact dwarf galaxies |
title_full |
Chemodynamics of blue compact dwarf galaxies |
title_fullStr |
Chemodynamics of blue compact dwarf galaxies |
title_full_unstemmed |
Chemodynamics of blue compact dwarf galaxies |
title_sort |
Chemodynamics 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 physical and chemical properties Blue Compact Dwarf galaxies |
topic |
Ciencias Astronómicas ionizing gas physical and chemical properties Blue Compact Dwarf galaxies |
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 LMFIT (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. Our 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 Hägele 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 LMFIT (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. Our 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 Hägele 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/10915/165265 |
url |
http://sedici.unlp.edu.ar/handle/10915/165265 |
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) |
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 189-193 |
dc.source.none.fl_str_mv |
reponame:SEDICI (UNLP) instname:Universidad Nacional de La Plata instacron:UNLP |
reponame_str |
SEDICI (UNLP) |
collection |
SEDICI (UNLP) |
instname_str |
Universidad Nacional de La Plata |
instacron_str |
UNLP |
institution |
UNLP |
repository.name.fl_str_mv |
SEDICI (UNLP) - Universidad Nacional de La Plata |
repository.mail.fl_str_mv |
alira@sedici.unlp.edu.ar |
_version_ |
1844616306106564608 |
score |
13.070432 |