Sökning: ((WFRF:(Lardo C.)) pers:(Alfaro E. J.) pers:(Bragaglia A.)) >
The Gaia-ESO Survey :
The Gaia-ESO Survey : Probes of the inner disk abundance gradient
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- Jacobson, H. R. (författare)
- MIT, Kavli Inst Astrophys & Space Res, 77 Massachusetts Ave, Cambridge, MA 02139 USA.,Massachusetts Institute of Technology
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- Friel, E. D. (författare)
- Indiana Univ, Dept Astron, Bloomington, IN 47405 USA.,Indiana University
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- Jilkova, L. (författare)
- Leiden Observ, POB 9513, NL-2300 RA Leiden, Netherlands.,Leiden University,University of Cambridge,Univ Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England.
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- Magrini, L. (författare)
- Osserv Astrofis Arcetri, INAF, Largo E Fermi 5, I-50125 Florence, Italy.,INAF - Osservatorio Astrofisico di Arcetri
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- Bragaglia, A. (författare)
- Osservatorio Astron Bologna, INAF, Via Ranzani 1, I-40127 Bologna, Italy.,INAF Osservatorio Astronomico di Bologna
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- Vallenari, A. (författare)
- Osserv Astron Padova, INAF, Vicolo Osservatorio 5, I-35122 Padua, Italy.,INAF - Osservatorio Astronomico di Padova
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- Tosi, M. (författare)
- Osservatorio Astron Bologna, INAF, Via Ranzani 1, I-40127 Bologna, Italy.,INAF Osservatorio Astronomico di Bologna,CSIC Instituto de Astrofísica de Andalucía (IAA),CSIC, Inst Astrofis Andalucia, Apdo 3004, E-18080 Granada, Spain.
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- Randich, S. (författare)
- Osserv Astrofis Arcetri, INAF, Largo E Fermi 5, I-50125 Florence, Italy.,INAF - Osservatorio Astrofisico di Arcetri,INAF - Osservatorio Astronomico di Padova,Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences,Osserv Astron Padova, INAF, Vicolo Osservatorio 5, I-35122 Padua, Italy.,Nicolaus Copernicus Astron Ctr, Dept Astrophys, Ul Rabianska 8, PL-87100 Torun, Poland.
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- Donati, P. (författare)
- Osservatorio Astron Bologna, INAF, Via Ranzani 1, I-40127 Bologna, Italy.;Dipartimento Fis & Astron, Via Ranzani 1, I-40127 Bologna, Italy.,University of Bologna
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- Cantat-Gaudin, T. (författare)
- Univ Padua, Dipartimento Fis & Astron, Vicolo Osservatorio 3, I-35122 Padua, Italy.,University of Padova,Vilnius University,Vilnius Univ, Inst Theoret Phys & Astron, A Gostauto 12, LT-01108 Vilnius, Lithuania.
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- Sordo, R. (författare)
- Osserv Astron Padova, INAF, Vicolo Osservatorio 5, I-35122 Padua, Italy.
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- Smiljanic, R. (författare)
- Nicolaus Copernicus Astron Ctr, Dept Astrophys, Ul Rabianska 8, PL-87100 Torun, Poland.
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- Overbeek, J. C. (författare)
- Indiana Univ, Dept Astron, Bloomington, IN 47405 USA.,Indiana University
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- Carraro, G. (författare)
- European So Observ, Alonso Cordova 3107 Vitacura, Santiago, Chile.,European Southern Observatory Santiago
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- Tautvaisiene, G. (författare)
- Vilnius Univ, Inst Theoret Phys & Astron, A Gostauto 12, LT-01108 Vilnius, Lithuania.
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- Roman, I. San (författare)
- Ctr Estudios Fis Cosmos Aragon, Plaza San Juan 1, Teruel 44001, Spain.,Centro de Estudios de Física del Cosmos de Aragón
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- Villanova, S. (författare)
- Univ Concepcion, Dept Astron, Casilla 160-C, Concepcion, Chile.,University of Concepción
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- Geisler, D. (författare)
- Univ Concepcion, Dept Astron, Casilla 160-C, Concepcion, Chile.
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- Munoz, C. (författare)
- Univ Concepcion, Dept Astron, Casilla 160-C, Concepcion, Chile.,University of Concepción
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- Jimenez-Esteban, F. (författare)
- Ctr Astrobiol INTA CSIC, Dpto Astrofis, POB 78, Madrid 28691, Spain.;Suffolk Univ, Madrid Campus,C Valle Vina 3, Madrid 28003, Spain.,Suffolk University,INAF Palermo Astronomical Observatory,INAF - Osservatorio Astrofisico di Arcetri,Osservatorio Astronom Palermo, INAF, Piazza Parlamento 1, I-90134 Palermo, Italy.,Osserv Astrofis Arcetri, INAF, Largo E Fermi 5, I-50125 Florence, Italy.
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- Bensby, T. (författare)
- Lund University,Lunds universitet,Astronomi - Genomgår omorganisation,Institutionen för astronomi och teoretisk fysik - Genomgår omorganisation,Naturvetenskapliga fakulteten,Lund Observatory - Undergoing reorganization,Department of Astronomy and Theoretical Physics - Undergoing reorganization,Faculty of Science,Univ Concepcion, Dept Astron, Casilla 160-C, Concepcion, Chile.,Lund Observ, Dept Astron & Theoret Phys, Box 43, S-22100 Lund, Sweden.
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- Gilmore, G. (författare)
- Univ Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England.,University of Cambridge,INAF - Osservatorio Astrofisico di Arcetri,University of Porto,Osserv Astrofis Arcetri, INAF, Largo E Fermi 5, I-50125 Florence, Italy.,Univ Porto, Inst Astrofis & Ciencias Espaco, CAUP, Rua Estrelas, P-4150762 Oporto, Portugal.
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- Alfaro, E. J. (författare)
- CSIC, Inst Astrofis Andalucia, Apdo 3004, E-18080 Granada, Spain.,CSIC Instituto de Astrofísica de Andalucía (IAA)
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- Bensby, T. (författare)
- Lund Observ, Dept Astron & Theoret Phys, Box 43, S-22100 Lund, Sweden.
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- Flaccomio, E. (författare)
- Osservatorio Astronom Palermo, INAF, Piazza Parlamento 1, I-90134 Palermo, Italy.
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- Koposov, S. E. (författare)
- Univ Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England.;Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Moscow 119992, Russia.,Sternberg Astronomical Institute
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- Korn, Andreas J. (författare)
- Uppsala University,Uppsala universitet,Teoretisk astrofysik
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- Pancino, E. (författare)
- Osserv Astrofis Arcetri, INAF, Largo E Fermi 5, I-50125 Florence, Italy.;ASI Sci Data Ctr, Via Politecn SNC, I-00133 Rome, Italy.,Italian Space Agency
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- Recio-Blanco, A. (författare)
- Univ Nice Sophia Antipolis, CNRS, Observ Cote Azur, Lab Lagrange UMR7293, CS 34229, F-06304 Nice 4, France.,Côte d'Azur Observatory
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- Casey, A. R. (författare)
- Univ Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England.,University of Cambridge
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- Costado, M. T. (författare)
- CSIC, Inst Astrofis Andalucia, Apdo 3004, E-18080 Granada, Spain.
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- Franciosini, E. (författare)
- Osserv Astrofis Arcetri, INAF, Largo E Fermi 5, I-50125 Florence, Italy.
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- Heiter, Ulrike (författare)
- Uppsala University,Uppsala universitet,Observationell astrofysik
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- Hill, V. (författare)
- Côte d'Azur Observatory
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- Hourihane, A. (författare)
- Univ Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England.,University of Cambridge
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- Lardo, C. (författare)
- Liverpool John Moores Univ, Astrophys Res Inst, 146 Brownlow Hill, Liverpool L3 5RF, Merseyside, England.,Liverpool John Moores University
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- de laverny, P. (författare)
- Univ Nice Sophia Antipolis, CNRS, Observ Cote Azur, Lab Lagrange UMR7293, CS 34229, F-06304 Nice 4, France.,Côte d'Azur Observatory
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- Lewis, J. (författare)
- Univ Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England.
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- Monaco, L. (författare)
- Univ Andres Bello Republ 220, Dept Ciencias Fis, Santiago, Chile.,Andrés Bello National University
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- Morbidelli, L. (författare)
- Osserv Astrofis Arcetri, INAF, Largo E Fermi 5, I-50125 Florence, Italy.,INAF - Osservatorio Astrofisico di Arcetri
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- Sacco, G. G. (författare)
- Osserv Astrofis Arcetri, INAF, Largo E Fermi 5, I-50125 Florence, Italy.
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- Sousa, S. G. (författare)
- Univ Porto, Inst Astrofis & Ciencias Espaco, CAUP, Rua Estrelas, P-4150762 Oporto, Portugal.
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- Worley, C. C. (författare)
- Univ Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England.,University of Cambridge
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- Zaggia, S. (författare)
- Osserv Astron Padova, INAF, Vicolo Osservatorio 5, I-35122 Padua, Italy.,INAF - Osservatorio Astronomico di Padova
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MIT, Kavli Inst Astrophys & Space Res, 77 Massachusetts Ave, Cambridge, MA 02139 USA Massachusetts Institute of Technology (creator_code:org_t)
- 2016-06-07
- 2016
- Engelska.
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Ingår i: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 591
- Relaterad länk:
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https://www.aanda.or...
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http://dx.doi.org/10...
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https://urn.kb.se/re...
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https://doi.org/10.1...
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https://lup.lub.lu.s...
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Abstract
Ämnesord
Stäng
- Context. The nature of the metallicity gradient inside the solar circle (R-GC < 8 kpc) is poorly understood, but studies of Cepheids and a small sample of open clusters suggest that it steepens in the inner disk. Aims. We investigate the metallicity gradient of the inner disk using a sample of inner disk open clusters that is three times larger than has previously been studied in the literature to better characterize the gradient in this part of the disk. Methods. We used the Gaia-ESO Survey (GES) [Fe/H] values and stellar parameters for stars in 12 open clusters in the inner disk from GES-UVES data. Cluster mean [Fe/H] values were determined based on a membership analysis for each cluster. Where necessary, distances and ages to clusters were determined via comparison to theoretical isochrones. Results. The GES open clusters exhibit a radial metallicity gradient of -0.10 +/- 0.02 dex kpc(-1), consistent with the gradient measured by other literature studies of field red giant stars and open clusters in the range R-GC similar to 6-12 kpc. We also measure a trend of increasing [Fe/H] with increasing cluster age, as has also been found in the literature. Conclusions. We find no evidence for a steepening of the inner disk metallicity gradient inside the solar circle as earlier studies indicated. The age-metallicity relation shown by the clusters is consistent with that predicted by chemical evolution models that include the effects of radial migration, but a more detailed comparison between cluster observations and models would be premature.
Ämnesord
- NATURVETENSKAP -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
- NATURAL SCIENCES -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
Nyckelord
- Galaxy: formation
- Galaxy: disk
- Galaxy: abundances
- stars: abundances
- Galaxy: abundances
- Galaxy: disk
- Galaxy: formation
- Stars: abundances
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- art (ämneskategori)
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Jacobson, H. R.
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Friel, E. D.
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Jilkova, L.
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Magrini, L.
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Bragaglia, A.
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Vallenari, A.
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visa fler...
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Tosi, M.
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Randich, S.
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Donati, P.
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Cantat-Gaudin, T ...
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Sordo, R.
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Smiljanic, R.
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Overbeek, J. C.
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Carraro, G.
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Tautvaisiene, G.
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Roman, I. San
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Villanova, S.
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Geisler, D.
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Munoz, C.
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Jimenez-Esteban, ...
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Bensby, T.
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Gilmore, G.
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Alfaro, E. J.
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Flaccomio, E.
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Koposov, S. E.
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Korn, Andreas J.
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Pancino, E.
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Recio-Blanco, A.
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Casey, A. R.
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Costado, M. T.
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Franciosini, E.
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Heiter, Ulrike
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Hill, V.
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Hourihane, A.
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Lardo, C.
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de laverny, P.
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Lewis, J.
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Monaco, L.
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Morbidelli, L.
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Sacco, G. G.
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Sousa, S. G.
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Worley, C. C.
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Zaggia, S.
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