Variability in NGC 3201 giant stars and its impact on their spectroscopic [Fe/H] determination
- Autores
- Llancaqueo Albornoz, Álvaro; Sandro, Villanova; Cortés, C. C.; Ahumada, Javier; Parisi, Maria Celeste
- Año de publicación
- 2021
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We present the analysis of 34 light curves in V and I of 17 giant stars in the globular cluster NGC 3201 to check if such stars are variable and if their variability has some kind of impact on the iron abundance as obtained from spectroscopic measurements. First, we computed the generalized Lomb-Scargle and phase dispersion minimization periodograms of the sample to check if the stars were variables. In this way, seven stars of the sample were found to be nonvariable, two stars are considered as possible variables, and eight stars were found to be variable, with periods ranging from 0.0881 ± 0.0001 to 0.5418 ± 0.0027 days. According to the literature, the variables have distinct values of [Fe I/H]: the three most metal-rich stars are in the red giant branch (RGB) stage, one has [Fe I/H] = -1.37 dex, while the other two have [Fe I/H] = -1.31 dex. The two most metal-poor variables have [Fe I/H] = -1.61 dex and [Fe I/H] = -1.62 dex, and are AGB stars; the remaining variables have [Fe I/H] = -1.44, -1.48, and -1.50 dex, the first two being RGB stars while the last is an AGB star. On the other hand, stars that appear to be nonvariable have -1.56 ≤ [Fe I/H] ≤ -1.40. We conclude that variability somehow affects the spectroscopic determination of the iron content of giant stars in NGC 3201, increasing the iron spread of the cluster. If variability is not taken into account, this spread could be incorrectly interpreted as due to an intrinsic iron spread affecting the stars of the cluster.
Fil: Llancaqueo Albornoz, Álvaro. Universidad de Concepción; Chile
Fil: Sandro, Villanova. Universidad de Concepción; Chile
Fil: Cortés, C. C.. Universidad de Concepción; Chile. Universidad del Bio Bio; Chile
Fil: Ahumada, Javier. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina
Fil: Parisi, Maria Celeste. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina - Materia
-
Globular star clusters
Stellar abundances
Solar and Stellar Astrophysics - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/173036
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Variability in NGC 3201 giant stars and its impact on their spectroscopic [Fe/H] determinationLlancaqueo Albornoz, ÁlvaroSandro, VillanovaCortés, C. C.Ahumada, JavierParisi, Maria CelesteGlobular star clustersStellar abundancesSolar and Stellar Astrophysicshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present the analysis of 34 light curves in V and I of 17 giant stars in the globular cluster NGC 3201 to check if such stars are variable and if their variability has some kind of impact on the iron abundance as obtained from spectroscopic measurements. First, we computed the generalized Lomb-Scargle and phase dispersion minimization periodograms of the sample to check if the stars were variables. In this way, seven stars of the sample were found to be nonvariable, two stars are considered as possible variables, and eight stars were found to be variable, with periods ranging from 0.0881 ± 0.0001 to 0.5418 ± 0.0027 days. According to the literature, the variables have distinct values of [Fe I/H]: the three most metal-rich stars are in the red giant branch (RGB) stage, one has [Fe I/H] = -1.37 dex, while the other two have [Fe I/H] = -1.31 dex. The two most metal-poor variables have [Fe I/H] = -1.61 dex and [Fe I/H] = -1.62 dex, and are AGB stars; the remaining variables have [Fe I/H] = -1.44, -1.48, and -1.50 dex, the first two being RGB stars while the last is an AGB star. On the other hand, stars that appear to be nonvariable have -1.56 ≤ [Fe I/H] ≤ -1.40. We conclude that variability somehow affects the spectroscopic determination of the iron content of giant stars in NGC 3201, increasing the iron spread of the cluster. If variability is not taken into account, this spread could be incorrectly interpreted as due to an intrinsic iron spread affecting the stars of the cluster.Fil: Llancaqueo Albornoz, Álvaro. Universidad de Concepción; ChileFil: Sandro, Villanova. Universidad de Concepción; ChileFil: Cortés, C. C.. Universidad de Concepción; Chile. Universidad del Bio Bio; ChileFil: Ahumada, Javier. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; ArgentinaFil: Parisi, Maria Celeste. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; ArgentinaIOP Publishing2021-02info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/173036Llancaqueo Albornoz, Álvaro; Sandro, Villanova; Cortés, C. C.; Ahumada, Javier; Parisi, Maria Celeste; Variability in NGC 3201 giant stars and its impact on their spectroscopic [Fe/H] determination; IOP Publishing; Astronomical Journal; 161; 2; 2-2021; 76-900004-62561538-3881CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-3881/abcf2finfo:eu-repo/semantics/altIdentifier/doi/10.3847/1538-3881/abcf2finfo:eu-repo/semantics/altIdentifier/arxiv/https://arxiv.org/abs/2012.00520info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:35:34Zoai:ri.conicet.gov.ar:11336/173036instacron: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 09:35:35.166CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Variability in NGC 3201 giant stars and its impact on their spectroscopic [Fe/H] determination |
title |
Variability in NGC 3201 giant stars and its impact on their spectroscopic [Fe/H] determination |
spellingShingle |
Variability in NGC 3201 giant stars and its impact on their spectroscopic [Fe/H] determination Llancaqueo Albornoz, Álvaro Globular star clusters Stellar abundances Solar and Stellar Astrophysics |
title_short |
Variability in NGC 3201 giant stars and its impact on their spectroscopic [Fe/H] determination |
title_full |
Variability in NGC 3201 giant stars and its impact on their spectroscopic [Fe/H] determination |
title_fullStr |
Variability in NGC 3201 giant stars and its impact on their spectroscopic [Fe/H] determination |
title_full_unstemmed |
Variability in NGC 3201 giant stars and its impact on their spectroscopic [Fe/H] determination |
title_sort |
Variability in NGC 3201 giant stars and its impact on their spectroscopic [Fe/H] determination |
dc.creator.none.fl_str_mv |
Llancaqueo Albornoz, Álvaro Sandro, Villanova Cortés, C. C. Ahumada, Javier Parisi, Maria Celeste |
author |
Llancaqueo Albornoz, Álvaro |
author_facet |
Llancaqueo Albornoz, Álvaro Sandro, Villanova Cortés, C. C. Ahumada, Javier Parisi, Maria Celeste |
author_role |
author |
author2 |
Sandro, Villanova Cortés, C. C. Ahumada, Javier Parisi, Maria Celeste |
author2_role |
author author author author |
dc.subject.none.fl_str_mv |
Globular star clusters Stellar abundances Solar and Stellar Astrophysics |
topic |
Globular star clusters Stellar abundances Solar and Stellar Astrophysics |
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 present the analysis of 34 light curves in V and I of 17 giant stars in the globular cluster NGC 3201 to check if such stars are variable and if their variability has some kind of impact on the iron abundance as obtained from spectroscopic measurements. First, we computed the generalized Lomb-Scargle and phase dispersion minimization periodograms of the sample to check if the stars were variables. In this way, seven stars of the sample were found to be nonvariable, two stars are considered as possible variables, and eight stars were found to be variable, with periods ranging from 0.0881 ± 0.0001 to 0.5418 ± 0.0027 days. According to the literature, the variables have distinct values of [Fe I/H]: the three most metal-rich stars are in the red giant branch (RGB) stage, one has [Fe I/H] = -1.37 dex, while the other two have [Fe I/H] = -1.31 dex. The two most metal-poor variables have [Fe I/H] = -1.61 dex and [Fe I/H] = -1.62 dex, and are AGB stars; the remaining variables have [Fe I/H] = -1.44, -1.48, and -1.50 dex, the first two being RGB stars while the last is an AGB star. On the other hand, stars that appear to be nonvariable have -1.56 ≤ [Fe I/H] ≤ -1.40. We conclude that variability somehow affects the spectroscopic determination of the iron content of giant stars in NGC 3201, increasing the iron spread of the cluster. If variability is not taken into account, this spread could be incorrectly interpreted as due to an intrinsic iron spread affecting the stars of the cluster. Fil: Llancaqueo Albornoz, Álvaro. Universidad de Concepción; Chile Fil: Sandro, Villanova. Universidad de Concepción; Chile Fil: Cortés, C. C.. Universidad de Concepción; Chile. Universidad del Bio Bio; Chile Fil: Ahumada, Javier. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina Fil: Parisi, Maria Celeste. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina |
description |
We present the analysis of 34 light curves in V and I of 17 giant stars in the globular cluster NGC 3201 to check if such stars are variable and if their variability has some kind of impact on the iron abundance as obtained from spectroscopic measurements. First, we computed the generalized Lomb-Scargle and phase dispersion minimization periodograms of the sample to check if the stars were variables. In this way, seven stars of the sample were found to be nonvariable, two stars are considered as possible variables, and eight stars were found to be variable, with periods ranging from 0.0881 ± 0.0001 to 0.5418 ± 0.0027 days. According to the literature, the variables have distinct values of [Fe I/H]: the three most metal-rich stars are in the red giant branch (RGB) stage, one has [Fe I/H] = -1.37 dex, while the other two have [Fe I/H] = -1.31 dex. The two most metal-poor variables have [Fe I/H] = -1.61 dex and [Fe I/H] = -1.62 dex, and are AGB stars; the remaining variables have [Fe I/H] = -1.44, -1.48, and -1.50 dex, the first two being RGB stars while the last is an AGB star. On the other hand, stars that appear to be nonvariable have -1.56 ≤ [Fe I/H] ≤ -1.40. We conclude that variability somehow affects the spectroscopic determination of the iron content of giant stars in NGC 3201, increasing the iron spread of the cluster. If variability is not taken into account, this spread could be incorrectly interpreted as due to an intrinsic iron spread affecting the stars of the cluster. |
publishDate |
2021 |
dc.date.none.fl_str_mv |
2021-02 |
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/11336/173036 Llancaqueo Albornoz, Álvaro; Sandro, Villanova; Cortés, C. C.; Ahumada, Javier; Parisi, Maria Celeste; Variability in NGC 3201 giant stars and its impact on their spectroscopic [Fe/H] determination; IOP Publishing; Astronomical Journal; 161; 2; 2-2021; 76-90 0004-6256 1538-3881 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/173036 |
identifier_str_mv |
Llancaqueo Albornoz, Álvaro; Sandro, Villanova; Cortés, C. C.; Ahumada, Javier; Parisi, Maria Celeste; Variability in NGC 3201 giant stars and its impact on their spectroscopic [Fe/H] determination; IOP Publishing; Astronomical Journal; 161; 2; 2-2021; 76-90 0004-6256 1538-3881 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-3881/abcf2f info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-3881/abcf2f info:eu-repo/semantics/altIdentifier/arxiv/https://arxiv.org/abs/2012.00520 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by/2.5/ar/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by/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 |
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CONICET Digital (CONICET) |
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Consejo Nacional de Investigaciones Científicas y Técnicas |
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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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13.070432 |