On the APOGEE DR14 sodium spread in the Galactic open cluster NGC188

Autores
Piatti, Andres Eduardo
Año de publicación
2019
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
[Na/Fe] is a flagship among chemical abundances as a good indicator of the existence of multiple populations in globular clusters, with spreads of up to 0.6 dex and more; no globular cluster having a null spread (Gratton et al. 2004; Bastian & Lardo 2018). As far as Galactic open clusters are considered, no multiple populations have been found yet (see, Bragaglia et al. 2012; Carrera & Mart´ınez-V´azquez 2013). Enter NGC 188 (age = 6.3±0.2 Gyr, Bonatto 2019). I made use of the publicly available Sloan Digital Sky Survey IV, in particular of APOGEE DR14 (Abolfathi et al. 2018) through the APOGEE Stellar Parameters and Abundances pipeline (ASPCAP, Garc´ıa P´erez et al. 2016), to search for stellar parameters and element abundances of stars in the field of NGC 188. As a result, I gathered 758 stars distributed within a radius of ∼ 1.6◦ from the cluster center and with 2MASS Ks mag down to ∼ 12.5 mag. In order to disentangle bonafide cluster members from field stars I used the diagnostic plane [Fe/H] vs. RV (see Fig. 1), which clearly highlights a group of stars tightly distributed around the known cluster with RV = 42.4±0.1 km/s (Chumak et al. 2010) and metal content 0.12 < [Fe/H] (dex) < 0.20 (Bonatto 2019)). They are red giant stars with 4100 . Tef f (K) . 5000 and 1.5 . log(g) . 3.5, distributed within a circle with a radius of 250 , which is nearly half of the cluster tidal radius (44.780 , Wang et al. 2015).
Fil: Piatti, Andres Eduardo. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Mendoza. Instituto Interdisciplinario de Ciencias Básicas. - Universidad Nacional de Cuyo. Instituto Interdisciplinario de Ciencias Básicas; Argentina
Materia
Cluster
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:11336/128356

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spelling On the APOGEE DR14 sodium spread in the Galactic open cluster NGC188Piatti, Andres EduardoClusterhttps://purl.org/becyt/ford/1.7https://purl.org/becyt/ford/1[Na/Fe] is a flagship among chemical abundances as a good indicator of the existence of multiple populations in globular clusters, with spreads of up to 0.6 dex and more; no globular cluster having a null spread (Gratton et al. 2004; Bastian & Lardo 2018). As far as Galactic open clusters are considered, no multiple populations have been found yet (see, Bragaglia et al. 2012; Carrera & Mart´ınez-V´azquez 2013). Enter NGC 188 (age = 6.3±0.2 Gyr, Bonatto 2019). I made use of the publicly available Sloan Digital Sky Survey IV, in particular of APOGEE DR14 (Abolfathi et al. 2018) through the APOGEE Stellar Parameters and Abundances pipeline (ASPCAP, Garc´ıa P´erez et al. 2016), to search for stellar parameters and element abundances of stars in the field of NGC 188. As a result, I gathered 758 stars distributed within a radius of ∼ 1.6◦ from the cluster center and with 2MASS Ks mag down to ∼ 12.5 mag. In order to disentangle bonafide cluster members from field stars I used the diagnostic plane [Fe/H] vs. RV (see Fig. 1), which clearly highlights a group of stars tightly distributed around the known cluster with RV = 42.4±0.1 km/s (Chumak et al. 2010) and metal content 0.12 < [Fe/H] (dex) < 0.20 (Bonatto 2019)). They are red giant stars with 4100 . Tef f (K) . 5000 and 1.5 . log(g) . 3.5, distributed within a circle with a radius of 250 , which is nearly half of the cluster tidal radius (44.780 , Wang et al. 2015).Fil: Piatti, Andres Eduardo. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Mendoza. Instituto Interdisciplinario de Ciencias Básicas. - Universidad Nacional de Cuyo. Instituto Interdisciplinario de Ciencias Básicas; ArgentinaAmerican Astronomical Society2019-07info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/128356Piatti, Andres Eduardo; On the APOGEE DR14 sodium spread in the Galactic open cluster NGC188; American Astronomical Society; Research Notes of the American Astronomical Society; 3; 7; 7-2019; 104-1052515-5172CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/arxiv/https://arxiv.org/abs/1907.10476info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/2515-5172/ab3417info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-29T12:23:28Zoai:ri.conicet.gov.ar:11336/128356instacron: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:34982025-10-29 12:23:28.925CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv On the APOGEE DR14 sodium spread in the Galactic open cluster NGC188
title On the APOGEE DR14 sodium spread in the Galactic open cluster NGC188
spellingShingle On the APOGEE DR14 sodium spread in the Galactic open cluster NGC188
Piatti, Andres Eduardo
Cluster
title_short On the APOGEE DR14 sodium spread in the Galactic open cluster NGC188
title_full On the APOGEE DR14 sodium spread in the Galactic open cluster NGC188
title_fullStr On the APOGEE DR14 sodium spread in the Galactic open cluster NGC188
title_full_unstemmed On the APOGEE DR14 sodium spread in the Galactic open cluster NGC188
title_sort On the APOGEE DR14 sodium spread in the Galactic open cluster NGC188
dc.creator.none.fl_str_mv Piatti, Andres Eduardo
author Piatti, Andres Eduardo
author_facet Piatti, Andres Eduardo
author_role author
dc.subject.none.fl_str_mv Cluster
topic Cluster
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.7
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv [Na/Fe] is a flagship among chemical abundances as a good indicator of the existence of multiple populations in globular clusters, with spreads of up to 0.6 dex and more; no globular cluster having a null spread (Gratton et al. 2004; Bastian & Lardo 2018). As far as Galactic open clusters are considered, no multiple populations have been found yet (see, Bragaglia et al. 2012; Carrera & Mart´ınez-V´azquez 2013). Enter NGC 188 (age = 6.3±0.2 Gyr, Bonatto 2019). I made use of the publicly available Sloan Digital Sky Survey IV, in particular of APOGEE DR14 (Abolfathi et al. 2018) through the APOGEE Stellar Parameters and Abundances pipeline (ASPCAP, Garc´ıa P´erez et al. 2016), to search for stellar parameters and element abundances of stars in the field of NGC 188. As a result, I gathered 758 stars distributed within a radius of ∼ 1.6◦ from the cluster center and with 2MASS Ks mag down to ∼ 12.5 mag. In order to disentangle bonafide cluster members from field stars I used the diagnostic plane [Fe/H] vs. RV (see Fig. 1), which clearly highlights a group of stars tightly distributed around the known cluster with RV = 42.4±0.1 km/s (Chumak et al. 2010) and metal content 0.12 < [Fe/H] (dex) < 0.20 (Bonatto 2019)). They are red giant stars with 4100 . Tef f (K) . 5000 and 1.5 . log(g) . 3.5, distributed within a circle with a radius of 250 , which is nearly half of the cluster tidal radius (44.780 , Wang et al. 2015).
Fil: Piatti, Andres Eduardo. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Mendoza. Instituto Interdisciplinario de Ciencias Básicas. - Universidad Nacional de Cuyo. Instituto Interdisciplinario de Ciencias Básicas; Argentina
description [Na/Fe] is a flagship among chemical abundances as a good indicator of the existence of multiple populations in globular clusters, with spreads of up to 0.6 dex and more; no globular cluster having a null spread (Gratton et al. 2004; Bastian & Lardo 2018). As far as Galactic open clusters are considered, no multiple populations have been found yet (see, Bragaglia et al. 2012; Carrera & Mart´ınez-V´azquez 2013). Enter NGC 188 (age = 6.3±0.2 Gyr, Bonatto 2019). I made use of the publicly available Sloan Digital Sky Survey IV, in particular of APOGEE DR14 (Abolfathi et al. 2018) through the APOGEE Stellar Parameters and Abundances pipeline (ASPCAP, Garc´ıa P´erez et al. 2016), to search for stellar parameters and element abundances of stars in the field of NGC 188. As a result, I gathered 758 stars distributed within a radius of ∼ 1.6◦ from the cluster center and with 2MASS Ks mag down to ∼ 12.5 mag. In order to disentangle bonafide cluster members from field stars I used the diagnostic plane [Fe/H] vs. RV (see Fig. 1), which clearly highlights a group of stars tightly distributed around the known cluster with RV = 42.4±0.1 km/s (Chumak et al. 2010) and metal content 0.12 < [Fe/H] (dex) < 0.20 (Bonatto 2019)). They are red giant stars with 4100 . Tef f (K) . 5000 and 1.5 . log(g) . 3.5, distributed within a circle with a radius of 250 , which is nearly half of the cluster tidal radius (44.780 , Wang et al. 2015).
publishDate 2019
dc.date.none.fl_str_mv 2019-07
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/11336/128356
Piatti, Andres Eduardo; On the APOGEE DR14 sodium spread in the Galactic open cluster NGC188; American Astronomical Society; Research Notes of the American Astronomical Society; 3; 7; 7-2019; 104-105
2515-5172
CONICET Digital
CONICET
url http://hdl.handle.net/11336/128356
identifier_str_mv Piatti, Andres Eduardo; On the APOGEE DR14 sodium spread in the Galactic open cluster NGC188; American Astronomical Society; Research Notes of the American Astronomical Society; 3; 7; 7-2019; 104-105
2515-5172
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/arxiv/https://arxiv.org/abs/1907.10476
info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/2515-5172/ab3417
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 American Astronomical Society
publisher.none.fl_str_mv American Astronomical Society
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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