English
 
Help Privacy Policy Disclaimer
  Advanced SearchBrowse

Item

ITEM ACTIONSEXPORT
  The Gaia-ESO survey: Calibrating a relationship between age and the [C/N] abundance ratio with open clusters

Casali, G., Magrini, L., Tognelli, E., Jackson, R., Jeffries, R. D., Lagarde, N., et al. (2019). The Gaia-ESO survey: Calibrating a relationship between age and the [C/N] abundance ratio with open clusters. Astronomy and Astrophysics, 629.

Item is

Basic

show hide
Genre: Journal Article

Files

show Files

Locators

show
hide
Description:
-

Creators

show
hide
 Creators:
Casali, G.1, Author
Magrini, L.1, Author
Tognelli, E.1, Author
Jackson, R.1, Author
Jeffries, R. D.1, Author
Lagarde, N.1, Author
Tautvaišienė, G.1, Author
Masseron, T.1, Author
Degl'Innocenti, S.1, Author
Prada Moroni, P. G.1, Author
Kordopatis, G.1, Author
Pancino, E.1, Author
Randich, S.1, Author
Feltzing, S.1, Author
Sahlholdt, C.1, Author
Spina, L.1, Author
Friel, E.1, Author
Roccatagliata, V.1, Author
Sanna, N.1, Author
Bragaglia, A.1, Author
Drazdauskas, A.1, AuthorMikolaitis, ≈†.1, AuthorMinkevičiūtė, R.1, AuthorStonkutė, E.1, AuthorChorniy, Y.1, AuthorBagdonas, V.1, AuthorJimenez-Esteban, F.1, AuthorMartell, S.1, AuthorVan der Swaelmen, M.1, AuthorGilmore, G.1, AuthorVallenari, A.1, AuthorBensby, T.1, AuthorKoposov, S. E.1, AuthorKorn, A.1, AuthorWorley, C.1, AuthorSmiljanic, R.1, AuthorBergemann, M.1, AuthorCarraro, G.1, AuthorDamiani, F.1, AuthorPrisinzano, L.1, AuthorBonito, R.1, AuthorFranciosini, E.1, AuthorGonneau, A.1, AuthorHourihane, A.1, AuthorJofre, P.1, AuthorLewis, J.1, AuthorMorbidelli, L.1, AuthorSacco, G.1, AuthorSousa, S. G.1, AuthorZaggia, S.1, AuthorLanzafame, A. C.1, AuthorHeiter, U.1, AuthorFrasca, A.1, AuthorBayo, A.1, Author more..
Affiliations:
1Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners, ou_2421692              

Content

show
hide
Free keywords: Galaxy: abundances open clusters and associations: general Galaxy: disk Astrophysics - Astrophysics of Galaxies
 Abstract: Context. In the era of large high-resolution spectroscopic surveys such as Gaia-ESO and APOGEE, high-quality spectra can contribute to our understanding of the Galactic chemical evolution by providing abundances of elements that belong to the different nucleosynthesis channels, and also by providing constraints to one of the most elusive astrophysical quantities: stellar age. <BR /> Aims: Some abundance ratios, such as [C/N], have been proven to be excellent indicators of stellar ages. We aim at providing an empirical relationship between stellar ages and [C/N] using open star clusters, observed by the Gaia-ESO and APOGEE surveys, as calibrators. <BR /> Methods: We used stellar parameters and abundances from the Gaia-ESO Survey and APOGEE Survey of the Galactic field and open cluster stars. Ages of star clusters were retrieved from the literature sources and validated using a common set of isochrones. We used the same isochrones to determine for each age and metallicity the surface gravity at which the first dredge-up and red giant branch bump occur. We studied the effect of extra-mixing processes in our sample of giant stars, and we derived the mean [C/N] in evolved stars, including only stars without evidence of extra mixing. By combining the Gaia-ESO and APOGEE samples of open clusters, we derived a linear relationship between [C/N] and (logarithmic) cluster ages. <BR /> Results: We apply our relationship to selected giant field stars in the Gaia-ESO and APOGEE surveys. We find an age separation between thin- and thick-disc stars and age trends within their populations, with an increasing age towards lower metallicity populations. <BR /> Conclusions: With this empirical relationship, we are able to provide an age estimate for giant stars in which C and N abundances are measured. For giant stars, the isochrone fitting method is indeed less sensitive than for dwarf stars at the turn-off. Our method can therefore be considered as an additional tool to give an independent estimate of the age of giant stars. The uncertainties in their ages is similar to those obtained using isochrone fitting for dwarf stars. Based on observations collected with the FLAMES instrument at VLT/UT2 telescope (Paranal Observatory, ESO, Chile), for the Gaia-ESO Large Public Spectroscopic Survey (188.B-3002, 193.B-0936).

Details

show
hide
Language(s):
 Dates: 2019
 Publication Status: Published in print
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Type: -
 Identifiers: -
 Degree: -

Event

show

Legal Case

show

Project information

show

Source 1

show
hide
Title: Astronomy and Astrophysics
Source Genre: Journal
 Creator(s):
Affiliations:
Publ. Info: -
Pages: - Volume / Issue: 629 Sequence Number: - Start / End Page: - Identifier: -