Sökning: WFRF:(Majewski S.) > (2020-2024) > Exploring the S-pro...
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000 | 07108naa a2200601 4500 | |
001 | oai:DiVA.org:mau-50500 | |
003 | SwePub | |
008 | 220308s2022 | |||||||||||000 ||eng| | |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:mau:diva-505002 URI |
024 | 7 | a https://doi.org/10.3847/1538-4357/ac42542 DOI |
040 | a (SwePub)mau | |
041 | a engb eng | |
042 | 9 SwePub | |
072 | 7 | a ref2 swepub-contenttype |
072 | 7 | a art2 swepub-publicationtype |
100 | 1 | a Sales-Silva, J. V.u Observatório Nacional/MCTIC, R. Gen. José Cristino, 77, 20921-400, Rio de Janeiro, Brazil4 aut |
245 | 1 0 | a Exploring the S-process History in the Galactic Disk :b Cerium Abundances and Gradients in Open Clusters from the OCCAM/APOGEE Sample |
264 | c 2022-02-21 | |
264 | 1 | b Institute of Physics (IOP),c 2022 |
338 | a electronic2 rdacarrier | |
520 | a The APOGEE Open Cluster Chemical Abundances and Mapping survey is used to probe the chemical evolution of the s-process element cerium in the Galactic disk. Cerium abundances were derived from measurements of Ce ii lines in the APOGEE spectra using the Brussels Automatic Code for Characterizing High Accuracy Spectra in 218 stars belonging to 42 open clusters. Our results indicate that, in general, for ages < 4 Gyr, younger open clusters have higher [Ce/Fe] and [Ce/α-element] ratios than older clusters. In addition, metallicity segregates open clusters in the [Ce/X]–age plane (where X can be H, Fe, or the α-elements O, Mg, Si, or Ca). These metallicity-dependent relations result in [Ce/Fe] and [Ce/α] ratios with ages that are not universal clocks. Radial gradients of [Ce/H] and [Ce/Fe] ratios in open clusters, binned by age, were derived for the first time, with d[Ce/H]/dRGC being negative, while d[Ce/Fe]/dRGC is positive. [Ce/H] and [Ce/Fe] gradients are approximately constant over time, with the [Ce/Fe] gradient becoming slightly steeper, changing by ∼+0.009 dex kpc−1 Gyr−1. Both the [Ce/H] and [Ce/Fe] gradients are shifted to lower values of [Ce/H] and [Ce/Fe] for older open clusters. The chemical pattern of Ce in open clusters across the Galactic disk is discussed within the context of s-process yields from asymptotic giant branch (AGB) stars, gigayear time delays in Ce enrichment of the interstellar medium, and the strong dependence of Ce nucleosynthesis on the metallicity of its AGB stellar sources. | |
650 | 7 | a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng |
700 | 1 | a Daflon, S.u Observatório Nacional/MCTIC, R. Gen. José Cristino, 77, 20921-400, Rio de Janeiro, Brazil4 aut |
700 | 1 | a Cunha, K.u Observatório Nacional/MCTIC, R. Gen. José Cristino, 77, 20921-400, Rio de Janeiro, Brazil; Steward Observatory, University of Arizona, Tucson, AZ 85719, USA4 aut |
700 | 1 | a Souto, D.u Departamento de Física, Universidade Federal de Sergipe, Av. Marechal Rondon, S/N, 49000-000 São Cristóvão, SE, Brazil4 aut |
700 | 1 | a Smith, V. V.u Noirlab, Tucson, AZ 85719, USA4 aut |
700 | 1 | a Chiappini, C.u Leibniz-Institut für Astrophysik Potsdam (AIP), An der Sternwarte 16, D-14482 Potsdam, Germany4 aut |
700 | 1 | a Donor, J.u Department of Physics & Astronomy, Texas Christian University, TCU Box 298840, Fort Worth, TX 76129, USA4 aut |
700 | 1 | a Frinchaboy, P. M.u Department of Physics & Astronomy, Texas Christian University, TCU Box 298840, Fort Worth, TX 76129, USA4 aut |
700 | 1 | a Garcia-Hernandez, D. A.u Instituto de Astrofísica de Canarias (IAC), E-38205 La Laguna, Tenerife, Spain; Universidad de La Laguna (ULL), Departamento de Astrofísica, E-38206 La Laguna, Tenerife, Spain4 aut |
700 | 1 | a Hayes, C.u Department of Astronomy, University of Washington, Box 351580, Seattle, WA 98195, USA4 aut |
700 | 1 | a Majewski, S. R.u Department of Astronomy, University of Virginia, Charlottesville, VA 22904-4325, USA4 aut |
700 | 1 | a Masseron, T.u Instituto de Astrofísica de Canarias (IAC), E-38205 La Laguna, Tenerife, Spain; Universidad de La Laguna (ULL), Departamento de Astrofísica, E-38206 La Laguna, Tenerife, Spain4 aut |
700 | 1 | a Schiavon, R. P.u Astrophysics Research Institute, Liverpool John Moores University, Liverpool, L3 5RF, UK4 aut |
700 | 1 | a Weinberg, D. H.u Department of Astronomy & Center for Cosmology and AstroParticle Physics, The Ohio State University, Columbus, OH 43210, USA; Institute for Advanced Study, Princeton, NJ 08540, USA4 aut |
700 | 1 | a Beaton, R. L.u The Carnegie Observatories, 813 Santa Barbara Street, Pasadena, CA 91101, USA4 aut |
700 | 1 | a Fernandez-Trincado, J. G.u Instituto de Astronomía, Universidad Católica del Norte, Av. Angamos 0610, Antofagasta, Chile; Instituto de Astronomía y Ciencias Planetarias, Universidad de Atacama, Copayapu 485, Copiapó, Chile4 aut |
700 | 1 | a Jönsson, Henriku Malmö universitet,Institutionen för materialvetenskap och tillämpad matematik (MTM)4 aut0 (Swepub:mau)ak0675 |
700 | 1 | a Lane, R. R.u Centro de Investigación en Astronomía, Universidad Bernardo O'Higgins, Avenida Viel 1497, Santiago, Chile4 aut |
700 | 1 | a Minniti, D.u Departamento de Ciencias Fisicas, Facultad de Ciencias Exactas, Universidad Andres Bello, Av. Fernandez Concha 700, Las Condes, Santiago, Chile; Vatican Observatory, I-00120 Vatican City State, Italy4 aut |
700 | 1 | a Manchado, A.u Instituto de Astrofísica de Canarias (IAC), E-38205 La Laguna, Tenerife, Spain; Universidad de La Laguna (ULL), Departamento de Astrofísica, E-38206 La Laguna, Tenerife, Spain; Instituto de Astrofísica de Canarias, C. Vía Láctea, s/n, 38205 San Cristóbal de La Laguna, Santa Cruz de Tenerife, Spain4 aut |
700 | 1 | a Moni Bidin, C.u Instituto de Astronomía, Universidad Católica del Norte, Av. Angamos 0610, Antofagasta, Chile4 aut |
700 | 1 | a Nitschelm, C.u Centro de Astronomía (CITEVA), Universidad de Antofagasta, Avenida Angamos 601, Antofagasta 1270300, Chile4 aut |
700 | 1 | a O'Connell, J.u Departamento de Astronomía, Casilla 160-C, Universidad de Concepción, Concepción, Chile4 aut |
700 | 1 | a Villanova, S.u Departamento de Astronomía, Casilla 160-C, Universidad de Concepción, Concepción, Chile4 aut |
710 | 2 | a Observatório Nacional/MCTIC, R. Gen. José Cristino, 77, 20921-400, Rio de Janeiro, Brazilb Observatório Nacional/MCTIC, R. Gen. José Cristino, 77, 20921-400, Rio de Janeiro, Brazil; Steward Observatory, University of Arizona, Tucson, AZ 85719, USA4 org |
773 | 0 | t Astrophysical Journald : Institute of Physics (IOP)g 926:2q 926:2x 0004-637Xx 1538-4357 |
856 | 4 | u https://doi.org/10.3847/1538-4357/ac4254y Fulltext |
856 | 4 | u https://mau.diva-portal.org/smash/get/diva2:1643052/FULLTEXT01.pdfx primaryx Raw objecty fulltext:print |
856 | 4 | u https://iopscience.iop.org/article/10.3847/1538-4357/ac4254/pdf |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:mau:diva-50500 |
856 | 4 8 | u https://doi.org/10.3847/1538-4357/ac4254 |
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