Ca II triplet spectroscopy of small magellanic cloud red giants. II. abundances for a sample of field stars

Autores
Parisi, Maria Celeste; Geisler, Doug; Grocholski, A. J.; Claria Olmedo, Juan Jose; Sarajedini, A.
Año de publicación
2015
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We have obtained metallicities of ∼360 red giant stars distributed in 15 Small Magellanic Cloud (SMC) fields from near-infrared spectra covering the Ca II triplet lines using the VLT + FORS2. The errors of the derived [Fe/H] values range from 0.09 to 0.35 dex per star, with a mean of 0.17 dex. The metallicity distribution (MD) of the whole sample shows a mean value of [Fe/H] = -1.00 ± 0.02, with a dispersion of 0.32 0.01, in agreement with global mean [Fe/H] values found in previous studies. We find no evidence of a metallicity gradient in the SMC. In fact, on analyzing the MD of each field, we derived mean values of [Fe/H] = -0.99 ± 0.08 and [Fe/H] = -1.02 ± 0.07 for fields located closer and farther than 4° from the center of the galaxy, respectively. In addition, there is a clear tendency for the field stars to be more metal-poor than the corresponding cluster they surround, independent of their positions in the galaxy and of the clusters' age. We argue that this most likely stems from the field stars being somewhat older and therefore somewhat more metal-poor than most of our clusters. © 2010. The American Astronomical Society.
Fil: Parisi, Maria Celeste. Universidad Nacional de Cordoba. Observatorio Astronomico de Cordoba; Argentina
Fil: Geisler, Doug. Universidad de Concepción; Chile
Fil: Grocholski, A. J.. University of Florida; Estados Unidos. Space Telescope Science Institute; Estados Unidos
Fil: Claria Olmedo, Juan Jose. Universidad Nacional de Cordoba. Observatorio Astronomico de Cordoba; Argentina
Fil: Sarajedini, A.. University of Florida; Estados Unidos
Materia
GALAXIES: STELLAR CONTENT
MAGELLANIC CLOUDS
STARS: ABUNDANCES
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:11336/59345

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spelling Ca II triplet spectroscopy of small magellanic cloud red giants. II. abundances for a sample of field starsParisi, Maria CelesteGeisler, DougGrocholski, A. J.Claria Olmedo, Juan JoseSarajedini, A.GALAXIES: STELLAR CONTENTMAGELLANIC CLOUDSSTARS: ABUNDANCEShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We have obtained metallicities of ∼360 red giant stars distributed in 15 Small Magellanic Cloud (SMC) fields from near-infrared spectra covering the Ca II triplet lines using the VLT + FORS2. The errors of the derived [Fe/H] values range from 0.09 to 0.35 dex per star, with a mean of 0.17 dex. The metallicity distribution (MD) of the whole sample shows a mean value of [Fe/H] = -1.00 ± 0.02, with a dispersion of 0.32 0.01, in agreement with global mean [Fe/H] values found in previous studies. We find no evidence of a metallicity gradient in the SMC. In fact, on analyzing the MD of each field, we derived mean values of [Fe/H] = -0.99 ± 0.08 and [Fe/H] = -1.02 ± 0.07 for fields located closer and farther than 4° from the center of the galaxy, respectively. In addition, there is a clear tendency for the field stars to be more metal-poor than the corresponding cluster they surround, independent of their positions in the galaxy and of the clusters' age. We argue that this most likely stems from the field stars being somewhat older and therefore somewhat more metal-poor than most of our clusters. © 2010. The American Astronomical Society.Fil: Parisi, Maria Celeste. Universidad Nacional de Cordoba. Observatorio Astronomico de Cordoba; ArgentinaFil: Geisler, Doug. Universidad de Concepción; ChileFil: Grocholski, A. J.. University of Florida; Estados Unidos. Space Telescope Science Institute; Estados UnidosFil: Claria Olmedo, Juan Jose. Universidad Nacional de Cordoba. Observatorio Astronomico de Cordoba; ArgentinaFil: Sarajedini, A.. University of Florida; Estados UnidosIOP Publishing2015-03info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/59345Parisi, Maria Celeste; Geisler, Doug; Grocholski, A. J.; Claria Olmedo, Juan Jose; Sarajedini, A.; Ca II triplet spectroscopy of small magellanic cloud red giants. II. abundances for a sample of field stars; IOP Publishing; Astronomical Journal; 139; 3; 3-2015; 1168-11770004-6256CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/0004-6256/139/3/1168/metainfo:eu-repo/semantics/altIdentifier/doi/10.1088/0004-6256/139/3/1168info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:33:51Zoai:ri.conicet.gov.ar:11336/59345instacron: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 09:33:51.87CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Ca II triplet spectroscopy of small magellanic cloud red giants. II. abundances for a sample of field stars
title Ca II triplet spectroscopy of small magellanic cloud red giants. II. abundances for a sample of field stars
spellingShingle Ca II triplet spectroscopy of small magellanic cloud red giants. II. abundances for a sample of field stars
Parisi, Maria Celeste
GALAXIES: STELLAR CONTENT
MAGELLANIC CLOUDS
STARS: ABUNDANCES
title_short Ca II triplet spectroscopy of small magellanic cloud red giants. II. abundances for a sample of field stars
title_full Ca II triplet spectroscopy of small magellanic cloud red giants. II. abundances for a sample of field stars
title_fullStr Ca II triplet spectroscopy of small magellanic cloud red giants. II. abundances for a sample of field stars
title_full_unstemmed Ca II triplet spectroscopy of small magellanic cloud red giants. II. abundances for a sample of field stars
title_sort Ca II triplet spectroscopy of small magellanic cloud red giants. II. abundances for a sample of field stars
dc.creator.none.fl_str_mv Parisi, Maria Celeste
Geisler, Doug
Grocholski, A. J.
Claria Olmedo, Juan Jose
Sarajedini, A.
author Parisi, Maria Celeste
author_facet Parisi, Maria Celeste
Geisler, Doug
Grocholski, A. J.
Claria Olmedo, Juan Jose
Sarajedini, A.
author_role author
author2 Geisler, Doug
Grocholski, A. J.
Claria Olmedo, Juan Jose
Sarajedini, A.
author2_role author
author
author
author
dc.subject.none.fl_str_mv GALAXIES: STELLAR CONTENT
MAGELLANIC CLOUDS
STARS: ABUNDANCES
topic GALAXIES: STELLAR CONTENT
MAGELLANIC CLOUDS
STARS: ABUNDANCES
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv We have obtained metallicities of ∼360 red giant stars distributed in 15 Small Magellanic Cloud (SMC) fields from near-infrared spectra covering the Ca II triplet lines using the VLT + FORS2. The errors of the derived [Fe/H] values range from 0.09 to 0.35 dex per star, with a mean of 0.17 dex. The metallicity distribution (MD) of the whole sample shows a mean value of [Fe/H] = -1.00 ± 0.02, with a dispersion of 0.32 0.01, in agreement with global mean [Fe/H] values found in previous studies. We find no evidence of a metallicity gradient in the SMC. In fact, on analyzing the MD of each field, we derived mean values of [Fe/H] = -0.99 ± 0.08 and [Fe/H] = -1.02 ± 0.07 for fields located closer and farther than 4° from the center of the galaxy, respectively. In addition, there is a clear tendency for the field stars to be more metal-poor than the corresponding cluster they surround, independent of their positions in the galaxy and of the clusters' age. We argue that this most likely stems from the field stars being somewhat older and therefore somewhat more metal-poor than most of our clusters. © 2010. The American Astronomical Society.
Fil: Parisi, Maria Celeste. Universidad Nacional de Cordoba. Observatorio Astronomico de Cordoba; Argentina
Fil: Geisler, Doug. Universidad de Concepción; Chile
Fil: Grocholski, A. J.. University of Florida; Estados Unidos. Space Telescope Science Institute; Estados Unidos
Fil: Claria Olmedo, Juan Jose. Universidad Nacional de Cordoba. Observatorio Astronomico de Cordoba; Argentina
Fil: Sarajedini, A.. University of Florida; Estados Unidos
description We have obtained metallicities of ∼360 red giant stars distributed in 15 Small Magellanic Cloud (SMC) fields from near-infrared spectra covering the Ca II triplet lines using the VLT + FORS2. The errors of the derived [Fe/H] values range from 0.09 to 0.35 dex per star, with a mean of 0.17 dex. The metallicity distribution (MD) of the whole sample shows a mean value of [Fe/H] = -1.00 ± 0.02, with a dispersion of 0.32 0.01, in agreement with global mean [Fe/H] values found in previous studies. We find no evidence of a metallicity gradient in the SMC. In fact, on analyzing the MD of each field, we derived mean values of [Fe/H] = -0.99 ± 0.08 and [Fe/H] = -1.02 ± 0.07 for fields located closer and farther than 4° from the center of the galaxy, respectively. In addition, there is a clear tendency for the field stars to be more metal-poor than the corresponding cluster they surround, independent of their positions in the galaxy and of the clusters' age. We argue that this most likely stems from the field stars being somewhat older and therefore somewhat more metal-poor than most of our clusters. © 2010. The American Astronomical Society.
publishDate 2015
dc.date.none.fl_str_mv 2015-03
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/11336/59345
Parisi, Maria Celeste; Geisler, Doug; Grocholski, A. J.; Claria Olmedo, Juan Jose; Sarajedini, A.; Ca II triplet spectroscopy of small magellanic cloud red giants. II. abundances for a sample of field stars; IOP Publishing; Astronomical Journal; 139; 3; 3-2015; 1168-1177
0004-6256
CONICET Digital
CONICET
url http://hdl.handle.net/11336/59345
identifier_str_mv Parisi, Maria Celeste; Geisler, Doug; Grocholski, A. J.; Claria Olmedo, Juan Jose; Sarajedini, A.; Ca II triplet spectroscopy of small magellanic cloud red giants. II. abundances for a sample of field stars; IOP Publishing; Astronomical Journal; 139; 3; 3-2015; 1168-1177
0004-6256
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/0004-6256/139/3/1168/meta
info:eu-repo/semantics/altIdentifier/doi/10.1088/0004-6256/139/3/1168
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 IOP Publishing
publisher.none.fl_str_mv IOP Publishing
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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