The star formation and chemical evolution history of the Fornax dwarf spheroidal galaxy

T. J L De Boer, E. Tolstoy, V. Hill, A. Saha, Edward W Olszewski, M. Mateo, E. Starkenburg, G. Battaglia, M. G. Walker

Research output: Contribution to journalArticle

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Abstract

We present deep photometry in the B, V and I filters from CTIO/MOSAIC for about 270 000 stars in the Fornax dwarf spheroidal galaxy, out to a radius of r ell ≈ 0.8 degrees. By combining the accurately calibrated photometry with the spectroscopic metallicity distributions of individual red giant branch stars we obtain the detailed star formation and chemical evolution history of Fornax. Fornax is dominated by intermediate age (1-10 Gyr) stellar populations, but also includes ancient (10-14 Gyr), and young (=1 Gyr) stars. We show that Fornax displays a radial age gradient, with younger, more metal-rich populations dominating the central region. This confirms results from previous works. Within an elliptical radius of 0.8 degrees, or 1.9 kpc from the centre, a total mass in stars of 4.3 × 10 7 M was formed, from the earliest times until 250 Myr ago. Using the detailed star formation history, age estimates are determined for individual stars on the upper RGB, for which spectroscopic abundances are available, giving an age-metallicity relation of the Fornax dSph from individual stars. This shows that the average metallicity of Fornax went up rapidly from [Fe/H] ≤-2.5 dex to [Fe/H] =-1.5 dex between 8-12 Gyr ago, after which a more gradual enrichment resulted in a narrow, well-defined sequence which reaches [Fe/H] ≈-0.8 dex, ≈3 Gyr ago. These ages also allow us to measure the build-up of chemical elements as a function of time, and thus determine detailed timescales for the evolution of individual chemical elements. A rapid decrease in [Mg/Fe] is seen for the stars with [Fe/H] ≥-1.5 dex, with a clear trend in age.

Original languageEnglish (US)
Article numberA73
JournalAstronomy and Astrophysics
Volume544
DOIs
StatePublished - 2012

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chemical evolution
dwarf galaxies
star formation
histories
stars
history
metallicity
chemical element
chemical elements
photometry
radii
chemical
filter
timescale
trends
metal
filters
gradients
estimates
metals

Keywords

  • Galaxies: dwarf
  • Galaxies: evolution
  • Galaxies: stellar content
  • Hertzsprung-Russell and C-M diagrams
  • Local Group

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

The star formation and chemical evolution history of the Fornax dwarf spheroidal galaxy. / De Boer, T. J L; Tolstoy, E.; Hill, V.; Saha, A.; Olszewski, Edward W; Mateo, M.; Starkenburg, E.; Battaglia, G.; Walker, M. G.

In: Astronomy and Astrophysics, Vol. 544, A73, 2012.

Research output: Contribution to journalArticle

De Boer, TJL, Tolstoy, E, Hill, V, Saha, A, Olszewski, EW, Mateo, M, Starkenburg, E, Battaglia, G & Walker, MG 2012, 'The star formation and chemical evolution history of the Fornax dwarf spheroidal galaxy', Astronomy and Astrophysics, vol. 544, A73. https://doi.org/10.1051/0004-6361/201219547
De Boer, T. J L ; Tolstoy, E. ; Hill, V. ; Saha, A. ; Olszewski, Edward W ; Mateo, M. ; Starkenburg, E. ; Battaglia, G. ; Walker, M. G. / The star formation and chemical evolution history of the Fornax dwarf spheroidal galaxy. In: Astronomy and Astrophysics. 2012 ; Vol. 544.
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KW - Hertzsprung-Russell and C-M diagrams

KW - Local Group

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