The Gaia -ESO survey: The non-universality of the age-chemical-clocks-metallicity relations in the Galactic disc

G. Casali; L. Spina; L. Magrini; A. I. Karakas; C. Kobayashi; A. R. Casey; S. Feltzing; M. Van Der Swaelmen; M. Tsantaki; P. Jofré; A. Bragaglia; D. Feuillet; T. Bensby; K. Biazzo; A. Gonneau; G. Tautvaišienė; M. Baratella; V. Roccatagliata; E. Pancino; S. Sousa; V. Adibekyan; S. Martell; A. Bayo; R. J. Jackson; R. D. Jeffries; G. Gilmore; S. Randich; E. Alfaro; S. E. Koposov; A. J. Korn; A. Recio-Blanco; R. Smiljanic; E. Franciosini; A. Hourihane; L. Monaco; L. Morbidelli; G. Sacco; C. Worley; S. Zaggia

doi:10.1051/0004-6361/202038055

The Gaia -ESO survey: The non-universality of the age-chemical-clocks-metallicity relations in the Galactic disc

G. Casali, L. Spina, L. Magrini, A. I. Karakas, C. Kobayashi, A. R. Casey, S. Feltzing, M. Van Der Swaelmen, M. Tsantaki, P. Jofré, A. Bragaglia, D. Feuillet, T. Bensby, K. Biazzo, A. Gonneau, G. Tautvaišienė, M. Baratella, V. Roccatagliata, E. Pancino, S. SousaV. Adibekyan, S. Martell, A. Bayo, R. J. Jackson, R. D. Jeffries, G. Gilmore, S. Randich, E. Alfaro, S. E. Koposov, A. J. Korn, A. Recio-Blanco, R. Smiljanic, E. Franciosini, A. Hourihane, L. Monaco, L. Morbidelli, G. Sacco, C. Worley, S. Zaggia

Research output: Contribution to journal › Article › peer-review

40 Citations (Scopus)

Original language	English
Article number	A127
Journal	Astronomy and Astrophysics
Volume	639
DOIs	https://doi.org/10.1051/0004-6361/202038055
Publication status	Published - 21 Jul 2020

Keywords

Galaxy: abundances
Galaxy: disk
Galaxy: evolution
Open clusters and associations: general
Stars: abundances

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

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10.1051/0004-6361/202038055

Cite this

Casali, G., Spina, L., Magrini, L., Karakas, A. I., Kobayashi, C., Casey, A. R., Feltzing, S., Van Der Swaelmen, M., Tsantaki, M., Jofré, P., Bragaglia, A., Feuillet, D., Bensby, T., Biazzo, K., Gonneau, A., Tautvaišienė, G., Baratella, M., Roccatagliata, V., Pancino, E., ... Zaggia, S. (2020). The Gaia -ESO survey: The non-universality of the age-chemical-clocks-metallicity relations in the Galactic disc. Astronomy and Astrophysics, 639, Article A127. https://doi.org/10.1051/0004-6361/202038055

@article{88f926b8437a48a79a3e284e719f9b72,

title = "The Gaia -ESO survey: The non-universality of the age-chemical-clocks-metallicity relations in the Galactic disc",

keywords = "Galaxy: abundances, Galaxy: disk, Galaxy: evolution, Open clusters and associations: general, Stars: abundances",

author = "G. Casali and L. Spina and L. Magrini and Karakas, {A. I.} and C. Kobayashi and Casey, {A. R.} and S. Feltzing and {Van Der Swaelmen}, M. and M. Tsantaki and P. Jofr{\'e} and A. Bragaglia and D. Feuillet and T. Bensby and K. Biazzo and A. Gonneau and G. Tautvai{\v s}ienė and M. Baratella and V. Roccatagliata and E. Pancino and S. Sousa and V. Adibekyan and S. Martell and A. Bayo and Jackson, {R. J.} and Jeffries, {R. D.} and G. Gilmore and S. Randich and E. Alfaro and Koposov, {S. E.} and Korn, {A. J.} and A. Recio-Blanco and R. Smiljanic and E. Franciosini and A. Hourihane and L. Monaco and L. Morbidelli and G. Sacco and C. Worley and S. Zaggia",

note = "Funding Information: Acknowledgements. We thank the referee for her/his useful and constructive comments and suggestions that improved our work. The authors would like to thanks Dr. Leslie K. Hunt for her help in the statistical interpretation of our results. Based on data products from observations made with ESO Telescopes at the La Silla Paranal Observatory under programme ID 188.B-3002. These data products have been processed by the Cambridge Astronomy Survey Unit (CASU) at the Institute of Astronomy, University of Cambridge, and by the FLAMES/UVES reduction team at INAF/Osservatorio Astrofisico di Arcetri. These data have been obtained from the GES Survey Data Archive, prepared and hosted by the Wide Field Astronomy Unit, Institute for Astronomy, University of Edinburgh, which is funded by the UK Science and Technology Facilities Council (STFC). This research has made use of the services of the ESO Science Archive Facility. This work was partly supported by the European Union FP7 programme through ERC grant number 320360 and by Funding Information: the Leverhulme Trust through grant RPG-2012-541. We acknowledge the support from INAF and Ministero dell{\textquoteright} Istruzione, dell{\textquoteright} Universit{\`a} e della Ricerca (MIUR) in the form of the grant “Premiale VLT 2012”. The results presented here benefit from discussions held during the GES workshops and conferences supported by the ESF (European Science Foundation) through the GREAT Research Network Programme. LM acknowledge the funding from the INAF PRIN-SKA 2017 program 1.05.01.88.04. LM and MVdS acknowledge the funding from MIUR Premiale 2016: MITIC. T.B. was supported by the project grant “The New Milky Way” from the Knut and Alice Wallenberg Foundation. M. acknowledges support provided by the Spanish Ministry of Economy and Competitiveness (MINECO), under grant AYA-2017-88254-P. L.S. acknowledges financial support from the Australian Research Council (Discovery Project 170100521) and from the Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), through project number CE170100013. F.J.E. acknowledges financial support from the ASTERICS project (ID:653477, H2020-EU.1.4.1.1. – Developing new world-class research infrastructures). U.H. acknowledges support from the Swedish National Space Agency (SNSA/Rymdstyrelsen). T.B was partly funded by the project grant “The New Milky Way” from the Knut and Alice Wallenberg Foundation, and partly by grant No. 2018-04857 from the Swedish Research Council. Funding Information: We thank the referee for her/his useful and constructive comments and suggestions that improved our work. The authors would like to thanks Dr. Leslie K. Hunt for her help in the statistical interpretation of our results. Based on data products from observations made with ESO Telescopes at the La Silla Paranal Observatory under programme ID 188.B-3002. These data products have been processed by the Cambridge Astronomy Survey Unit (CASU) at the Institute of Astronomy, University of Cambridge, and by the FLAMES/UVES reduction team at INAF/Osservatorio Astrofisico di Arcetri. These data have been obtained from the GES Survey Data Archive, prepared and hosted by the Wide Field Astronomy Unit, Institute for Astronomy, University of Edinburgh, which is funded by the UK Science and Technology Facilities Council (STFC). This research has made use of the services of the ESO Science Archive Facility. This work was partly supported by the European Union FP7 programme through ERC grant number 320360 and by the Leverhulme Trust through grant RPG-2012-541. We acknowledge the support from INAF and Ministero dell' Istruzione, dell' Universit? e della Ricerca (MIUR) in the form of the grant {"}Premiale VLT 2012{"}. The results presented here benefit from discussions held during the GES workshops and conferences supported by the ESF (European Science Foundation) through the GREAT Research Network Programme. LM acknowledge the funding from the INAF PRIN-SKA 2017 program 1.05.01.88.04. LM and MVdS acknowledge the funding from MIUR Premiale 2016: MITIC. T.B. was supported by the project grant {"}The New Milky Way{"} from the Knut and Alice Wallenberg Foundation. M. acknowledges support provided by the Spanish Ministry of Economy and Competitiveness (MINECO), under grant AYA-2017-88254-P. L.S. acknowledges financial support from the Australian Research Council (Discovery Project 170100521) and from the Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), through project number CE170100013. F.J.E. acknowledges financial support from the ASTERICS project (ID:653477, H2020-EU.1.4.1.1. - Developing new world-class research infrastructures). U.H. acknowledges support from the Swedish National Space Agency (SNSA/Rymdstyrelsen). T.B was partly funded by the project grant {"}The New Milky Way{"} from the Knut and Alice Wallenberg Foundation, and partly by grant No. 2018-04857 from the Swedish Research Council. Publisher Copyright: {\textcopyright} ESO 2020.",

year = "2020",

month = jul,

day = "21",

doi = "10.1051/0004-6361/202038055",

language = "English",

volume = "639",

journal = "Astronomy and Astrophysics",

issn = "0004-6361",

publisher = "EDP Sciences",

}

Casali, G, Spina, L, Magrini, L, Karakas, AI, Kobayashi, C, Casey, AR, Feltzing, S, Van Der Swaelmen, M, Tsantaki, M, Jofré, P, Bragaglia, A, Feuillet, D, Bensby, T, Biazzo, K, Gonneau, A, Tautvaišienė, G, Baratella, M, Roccatagliata, V, Pancino, E, Sousa, S, Adibekyan, V, Martell, S, Bayo, A, Jackson, RJ, Jeffries, RD, Gilmore, G, Randich, S, Alfaro, E, Koposov, SE, Korn, AJ, Recio-Blanco, A, Smiljanic, R, Franciosini, E, Hourihane, A, Monaco, L, Morbidelli, L, Sacco, G, Worley, C & Zaggia, S 2020, 'The Gaia -ESO survey: The non-universality of the age-chemical-clocks-metallicity relations in the Galactic disc', Astronomy and Astrophysics, vol. 639, A127. https://doi.org/10.1051/0004-6361/202038055

TY - JOUR

T1 - The Gaia -ESO survey

T2 - The non-universality of the age-chemical-clocks-metallicity relations in the Galactic disc

AU - Casali, G.

AU - Spina, L.

AU - Magrini, L.

AU - Karakas, A. I.

AU - Kobayashi, C.

AU - Casey, A. R.

AU - Feltzing, S.

AU - Van Der Swaelmen, M.

AU - Tsantaki, M.

AU - Jofré, P.

AU - Bragaglia, A.

AU - Feuillet, D.

AU - Bensby, T.

AU - Biazzo, K.

AU - Gonneau, A.

AU - Tautvaišienė, G.

AU - Baratella, M.

AU - Roccatagliata, V.

AU - Pancino, E.

AU - Sousa, S.

AU - Adibekyan, V.

AU - Martell, S.

AU - Bayo, A.

AU - Jackson, R. J.

AU - Jeffries, R. D.

AU - Gilmore, G.

AU - Randich, S.

AU - Alfaro, E.

AU - Koposov, S. E.

AU - Korn, A. J.

AU - Recio-Blanco, A.

AU - Smiljanic, R.

AU - Franciosini, E.

AU - Hourihane, A.

AU - Monaco, L.

AU - Morbidelli, L.

AU - Sacco, G.

AU - Worley, C.

AU - Zaggia, S.

N1 - Funding Information: Acknowledgements. We thank the referee for her/his useful and constructive comments and suggestions that improved our work. The authors would like to thanks Dr. Leslie K. Hunt for her help in the statistical interpretation of our results. Based on data products from observations made with ESO Telescopes at the La Silla Paranal Observatory under programme ID 188.B-3002. These data products have been processed by the Cambridge Astronomy Survey Unit (CASU) at the Institute of Astronomy, University of Cambridge, and by the FLAMES/UVES reduction team at INAF/Osservatorio Astrofisico di Arcetri. These data have been obtained from the GES Survey Data Archive, prepared and hosted by the Wide Field Astronomy Unit, Institute for Astronomy, University of Edinburgh, which is funded by the UK Science and Technology Facilities Council (STFC). This research has made use of the services of the ESO Science Archive Facility. This work was partly supported by the European Union FP7 programme through ERC grant number 320360 and by Funding Information: the Leverhulme Trust through grant RPG-2012-541. We acknowledge the support from INAF and Ministero dell’ Istruzione, dell’ Università e della Ricerca (MIUR) in the form of the grant “Premiale VLT 2012”. The results presented here benefit from discussions held during the GES workshops and conferences supported by the ESF (European Science Foundation) through the GREAT Research Network Programme. LM acknowledge the funding from the INAF PRIN-SKA 2017 program 1.05.01.88.04. LM and MVdS acknowledge the funding from MIUR Premiale 2016: MITIC. T.B. was supported by the project grant “The New Milky Way” from the Knut and Alice Wallenberg Foundation. M. acknowledges support provided by the Spanish Ministry of Economy and Competitiveness (MINECO), under grant AYA-2017-88254-P. L.S. acknowledges financial support from the Australian Research Council (Discovery Project 170100521) and from the Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), through project number CE170100013. F.J.E. acknowledges financial support from the ASTERICS project (ID:653477, H2020-EU.1.4.1.1. – Developing new world-class research infrastructures). U.H. acknowledges support from the Swedish National Space Agency (SNSA/Rymdstyrelsen). T.B was partly funded by the project grant “The New Milky Way” from the Knut and Alice Wallenberg Foundation, and partly by grant No. 2018-04857 from the Swedish Research Council. Funding Information: We thank the referee for her/his useful and constructive comments and suggestions that improved our work. The authors would like to thanks Dr. Leslie K. Hunt for her help in the statistical interpretation of our results. Based on data products from observations made with ESO Telescopes at the La Silla Paranal Observatory under programme ID 188.B-3002. These data products have been processed by the Cambridge Astronomy Survey Unit (CASU) at the Institute of Astronomy, University of Cambridge, and by the FLAMES/UVES reduction team at INAF/Osservatorio Astrofisico di Arcetri. These data have been obtained from the GES Survey Data Archive, prepared and hosted by the Wide Field Astronomy Unit, Institute for Astronomy, University of Edinburgh, which is funded by the UK Science and Technology Facilities Council (STFC). This research has made use of the services of the ESO Science Archive Facility. This work was partly supported by the European Union FP7 programme through ERC grant number 320360 and by the Leverhulme Trust through grant RPG-2012-541. We acknowledge the support from INAF and Ministero dell' Istruzione, dell' Universit? e della Ricerca (MIUR) in the form of the grant "Premiale VLT 2012". The results presented here benefit from discussions held during the GES workshops and conferences supported by the ESF (European Science Foundation) through the GREAT Research Network Programme. LM acknowledge the funding from the INAF PRIN-SKA 2017 program 1.05.01.88.04. LM and MVdS acknowledge the funding from MIUR Premiale 2016: MITIC. T.B. was supported by the project grant "The New Milky Way" from the Knut and Alice Wallenberg Foundation. M. acknowledges support provided by the Spanish Ministry of Economy and Competitiveness (MINECO), under grant AYA-2017-88254-P. L.S. acknowledges financial support from the Australian Research Council (Discovery Project 170100521) and from the Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), through project number CE170100013. F.J.E. acknowledges financial support from the ASTERICS project (ID:653477, H2020-EU.1.4.1.1. - Developing new world-class research infrastructures). U.H. acknowledges support from the Swedish National Space Agency (SNSA/Rymdstyrelsen). T.B was partly funded by the project grant "The New Milky Way" from the Knut and Alice Wallenberg Foundation, and partly by grant No. 2018-04857 from the Swedish Research Council. Publisher Copyright: © ESO 2020.

PY - 2020/7/21

Y1 - 2020/7/21

KW - Galaxy: abundances

KW - Galaxy: disk

KW - Galaxy: evolution

KW - Open clusters and associations: general

KW - Stars: abundances

UR - http://www.scopus.com/inward/record.url?scp=85089306480&partnerID=8YFLogxK

U2 - 10.1051/0004-6361/202038055

DO - 10.1051/0004-6361/202038055

M3 - Article

AN - SCOPUS:85089306480

SN - 0004-6361

VL - 639

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

M1 - A127

ER -

The Gaia -ESO survey: The non-universality of the age-chemical-clocks-metallicity relations in the Galactic disc

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