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
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/128356
Ver los metadatos del registro completo
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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 |
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2019-07 |
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info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
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article |
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publishedVersion |
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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 |
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http://hdl.handle.net/11336/128356 |
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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 |
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eng |
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eng |
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American Astronomical Society |
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American Astronomical Society |
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dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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