Estimating stellar ages and metallicities from parallaxes and broadband photometry: Successes and shortcomings

Forskningsoutput: TidskriftsbidragArtikel i vetenskaplig tidskrift

Abstract

A deep understanding of the Milky Way galaxy, its formation and evolution requires observations of huge numbers of stars. Stellar photometry, therefore, provides an economical method to obtain intrinsic stellar parameters. With the addition of distance information - a prospect made real for more than a billion stars with the second Gaia data release - deriving reliable ages from photometry is a possibility. We have developed a Bayesian method that generates 2D probability maps of a star's age and metallicity from photometry and parallax using isochrones. Our synthetic tests show that including a near-UV passband enables us to break the degeneracy between a star's age and metallicity for certain evolutionary stages. It is possible to find well-constrained ages and metallicities for turn-off and sub-giant stars with colours including a U band and a parallax with uncertainty less than ∼20%. Metallicities alone are possible for the main sequence and giant branch. We find good agreement with the literature when we apply our method to the Gaia benchmark stars, particularly for turn-off and young stars. Further tests on the old open cluster NGC 188, however, reveal significant limitations in the stellar isochrones. The ages derived for the cluster stars vary with evolutionary stage, such that turn-off ages disagree with those on the sub-giant branch, and metallicities vary significantly throughout. Furthermore, the parameters vary appreciably depending on which colour combinations are used in the derivation. We identify the causes of these mismatches and show that improvements are needed in the modelling of giant branch stars and in the creation and calibration of synthetic near-UV photometry. Our results warn against applying isochrone fitting indiscriminately. In particular, the uncertainty on the stellar models should be quantitatively taken into account. Further efforts to improve the models will result in significant advancements in our ability to study the Galaxy.

Detaljer

Författare
Enheter & grupper
Forskningsområden

Ämnesklassifikation (UKÄ) – OBLIGATORISK

  • Astronomi, astrofysik och kosmologi

Nyckelord

Originalspråkengelska
ArtikelnummerA27
TidskriftAstronomy and Astrophysics
Volym622
StatusPublished - 2019 feb 1
PublikationskategoriForskning
Peer review utfördJa

Relaterad forskningsoutput

Christian L. Sahlholdt, Sofia Feltzing, Lennart Lindegren & Ross P. Church, 2019, I : Monthly Notices of the Royal Astronomical Society. 482, 1, s. 895-920 26 s.

Forskningsoutput: TidskriftsbidragArtikel i vetenskaplig tidskrift

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Related projects

Sofia Feltzing, Thomas Bensby, Lennart Lindegren, Ross Church, Louise Howes, David Hobbs, Nils Ryde, Henrik Hartman, Paul Mcmillan & Edita Stonkute

Knut and Alice Wallenberg Foundation

2014/07/012027/06/30

Projekt: Forskning

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Relaterade aktiviteter

Feltzing, S. (Första/primär/huvudhandledare)
2015 aug 12019 feb 28

Aktivitet: Examination och handledarskapHandledning av postdoc

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