Near-infrared observations of the Fornax dwarf galaxy. I. The red giant branch
arXiv:astro-ph/0703489 · doi:10.1051/0004-6361:20066788
Abstract
We present a study of the evolved stellar populations in the dwarf spheroidal galaxy Fornax based on JHK imaging photometry. The observations cover an 18.5x18.5 arcmin central area with a mosaic of NTT/SOFI images. Our data sample all the red giant branch for the whole area. Deeeper observations reaching the red clump of helium-burning stars have also been obtained for a 4.5 x 4.5 arcmin region. Near-infrared photometry led to measurements of the distance to Fornax based on the K-band location of the RGB tip and the red clump. Once corrected for the mean age of the stellar populations in the galaxy, the derived distance modulus is 20.74 corresponding to a distance of 141 Kpc, in good agreement with estimates from optical data. By taking age effects into account, we have derived a distribution function of global metallicity [M/H] from optical-infrared colors of individual stars. Our photometric Metallicity Distribution Function covers the range -2.0<[M/H]<-0.6, with a main peak at [M/H]~-0.9 and a long tail of metal-poor stars, and less metal-rich stars than derived by recent spectroscopy. If metallicities from CaII triplet lines are correct, this result confirms a scenario of enhanced metal enrichment in the last 1-4 Gyr.
arXiv commentaccepted for publication in Astronomy and Astrophysics
References in corpus (28)
- Dwarf Galaxies of the Local Group
- A large stellar evolution database for population synthesis studies. I. Scaled solar models and isochrones
- Theoretical isochrones in several photometric systems I. Johnson-Cousins-Glass, HST/WFPC2, HST/NICMOS, Washington, and ESO Imaging Survey filter sets
- Color Transformations for the 2MASS Second Incremental Data Release
- Abundances for Globular Cluster Giants: I. Homogeneous Metallicities for 24 Clusters
- VLT/UVES Abundances in Four Nearby Dwarf Spheroidal Galaxies: I. Nucleosynthesis and Abundance Ratios
- Age and Metallicity Distribution of the Galactic Bulge from Extensive Optical and Near-IR Stellar Photometry
- The DART imaging and CaT survey of the Fornax Dwarf Spheroidal Galaxy
- A Comparison of Elemental Abundance Ratios in Globular Clusters, Field Stars, and Dwarf Spheroidal Galaxies
- VLT/UVES Abundances in Four Nearby Dwarf Spheroidal Galaxies: II. Implications for Understanding Galaxy Evolution
- K-Band Calibration of the Red Clump Luminosity
- Population effects on the red giant clump absolute magnitude: The K-band
- Tip of the Red Giant Branch Distances. I. Optimization of a Maximum Likelihood Algorithm
- WIYN Open Cluster Study. X. The K-Band Magnitude of the Red Clump as a Distance Indicator
- Using the Ca II Triplet to Trace Abundance Variations in Individual Red Giant Branch stars in Three Nearby Galaxies
- The Red Giant Branch in the Near-Infrared Colour-Magnitude Diagrams. I: The calibration of photometric indices
- An abundance analysis for four Red Horizontal Branch Stars in the extremely metal rich globular cluster NGC 6528
- The Red Giant Branch in Near-Infrared Colour-Magnitude Diagrams. II: The luminosity of the Bump and the Tip
- The Chemical Enrichment History of the Fornax Dwarf Spheroidal Galaxy from the Infrared Calcium Triplet
- Variable Stars in the Fornax Dwarf Galaxy
- The Age Dependent Luminosities of the Red Giant Branch Bump, Asymptotic Giant Branch Bump, and Horizontal Branch Red Clump
- Tip of the Red Giant Branch distances to galaxies with composite stellar populations
- Observational discovery of the AGB-bump in densely populated color-magnitude diagrams of galaxies and star clusters
- V, J, H and K Imaging of the Metal Rich Globular Cluster NGC 6528
- The Sagittarius dwarf irregular galaxy: metallicity and stellar populations
- Neutral Hydrogen Clouds near Early-Type Dwarf Galaxies of the Local Group
- Improved Searches for HI in Three Dwarf Spheroidal Galaxies
- Stellar Populations in the Local Group of Galaxies
Cited by in corpus (36)
- The Kinematics of the Ultra-Faint Milky Way Satellites: Solving the Missing Satellite Problem
- The Universal Stellar Mass-Stellar Metallicity Relation for Dwarf Galaxies
- The UKIDSS Galactic Plane Survey
- A high resolution VLT/FLAMES study of individual stars in the centre of the Fornax dwarf spheroidal galaxy
- Multi-Element Abundance Measurements from Medium-Resolution Spectra. IV. Alpha Element Distributions in Milky Way Dwarf Satellite Galaxies
- The Space Motion of Leo I: Hubble Space Telescope Proper Motion and Implied Orbit
- A large stellar evolution database for population synthesis studies. IV. Integrated properties and spectra
- Final Targeting Strategy for the SDSS-IV APOGEE-2S Survey
- VLT/FLAMES spectroscopy of red giant branch stars in the Fornax dwarf spheroidal galaxy
- AGB Stars in the Fornax Dwarf Spheroidal Galaxy
- Resolved Near-Infrared Stellar Populations in Nearby Galaxies
- The distance to the Fornax Dwarf Spheroidal Galaxy
- Near-Infrared Photometry of Globular Clusters Towards the Galactic Bulge: Observations and Photometric Metallicity Indicators
- The Araucaria Project. Infrared TRGB distances to the Carina and Fornax dwarf spheroidal galaxies
- Variable stars in the Fornax dSph Galaxy. II. Pulsating stars below the horizontal branch
- Spitzer Space Telescope spectral observations of AGB stars in the Fornax dwarf spheroidal galaxy
- Metallicity Evolution of the Six Most Luminous M31 Dwarf Satellites
- The VMC Survey. VIII. First results for Anomalous Cepheids
- The evolved stars of Leo II dSph galaxy from near-infrared UKIRT/WFCAM observations
- New constraints on the chemical evolution of the dwarf spheroidal galaxy LeoI from VLT spectroscopy
- The Near-Infrared Tip of the Red Giant Branch. I. A Calibration in the Isolated Dwarf Galaxy IC 1613
- Astrophysical Distance Scale II. Application of the JAGB Method: A Nearby Galaxy Sample
- On the relation between metallicity and RGB color in HST/ACS data
- Toward the general RGB slope-metallicity-age calibration: I Metallicities, Ages and Kinematics for Eight LMC Clusters
- Spectroscopic versus Photometric Metallicities: Milky Way Dwarf Spheroidal Companions as a Test Case
- The Araucaria Project. Infrared Tip of the Red Giant Branch Distances to Five Dwarf Galaxies in the Local Group
- The Araucaria Project: The distance to the Fornax Dwarf Galaxy from near-infrared photometry of RR Lyrae stars
- Near-Infrared photometry of carbon stars in the Sagittarius dwarf irregular galaxy and DDO 210
- Resolving Stellar Populations outside the Local Group: MAD observations of UKS2323-326
- Near-infrared spectroscopy of AGB star candidates in Fornax, Sculptor and NGC 6822
- The Asymptotic Giant Branch and the Tip of the Red Giant Branch as Probes of Star Formation History: The Nearby Dwarf Irregular Galaxy KKH 98
- Distances to Local Group Galaxies via Population II, Stellar Distance Indicators. II. The Fornax Dwarf Spheroidal
- A near-infrared study of AGB and red giant stars in the Leo I dSph galaxy
- The VMC Survey - XXXIII. The tip of the red giant branch in the Magellanic Clouds
- Population gradients and photometric metallicities in early- and transition-type dwarf galaxies: Clues from the Sculptor group
- Prospects of Stellar Abundance Studies from Near-IR Spectra Observed with the E-ELT