Insights from the outskirts: Chemical and dynamical properties in the outer parts of the Fornax dwarf spheroidal galaxy

Benjamin Hendricks*, Andreas Koch, Matthew Walker, Christian I. Johnson, Jorge Penarrubia, Gerard Gilmore

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

Abstract / Description of output

We present radial velocities and [Fe/H] abundances for 340 stars in the Fornax dwarf spheroidal from R similar to 16 000 spectra. The targets were obtained in the outer parts of the galaxy, a region that has been poorly studied. Our sample shows a wide range in [Fe/H], between -0.5 and -3.0 dex, in which we detect three subgroups. Removal of stars belonging to the most metal-rich population produces a truncated metallicity distribution function that is identical to Sculptor, indicating that these systems shared a similar early evolution, except that Fornax experienced a late, intense period of star formation (SF). The derived age-metallicity relation shows a fast increase in [Fe/H] at early ages, after which the enrichment flattens significantly for stars younger than similar to 8Gyr. Additionally, the data indicate a strong population of stars around 4Gyr, followed by a second rapid enrichment in [Fe/H]. A leaky-box chemical enrichment model generally matches the observed relation but predicts neither a significant population of young stars nor strong enrichment at late times. The young population in Fornax may therefore stem from an externally triggered SF event. Our dynamical analysis reveals an increasing velocity dispersion with decreasing [Fe/H] from sigma(sys) approximate to 7.5 km s(-1) to >= 14 km s(-1). The large velocity dispersion at low metallicities is possibly the result of a non-Gaussian velocity distribution among stars older than similar to 8 Gyr. Our sample also includes members from the Fornax globular clusters H2 and H5. In agreement with past studies we find [Fe/H] = -2.04 +/- 0.04 and a mean radial velocity RV = 59.36 +/- 0.31 km s(-1) for H2 and [Fe/H] = -2.02 +/- 0.11 and RV = 59.39 +/- 0.44 km s(-1) for H5. Finally, we test different calibrations of the calcium triplet over more than 2 dex in [Fe/H] and find best agreement with the calibration equations provided by Carrera et al. (2013, MNRAS, 434, 1681). Overall, we find high complexity in the chemical and dynamical properties, with signatures that additionally vary with galactocentric distance. Detailed knowledge about the properties of stars at all radii is therefore needed to draw a conclusive picture about the star formation and chemical evolution in Fornax.

Original languageEnglish
Article number82
Number of pages19
JournalAstronomy & Astrophysics
Publication statusPublished - Dec 2014

Keywords / Materials (for Non-textual outputs)

  • galaxies: individual: Fornax
  • galaxies: abundances
  • galaxies: evolution
  • galaxies: dwarf
  • galaxies: stellar content
  • galaxies: kinematics and dynamics


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