The calibration of the RGB Tip as a Standard Candle: Extension to Near Infrared colors and higher metallicity
arXiv:astro-ph/0404572 · doi:10.1051/0004-6361:20035910
Abstract
New empirical calibrations of the Red Giant Branch Tip in the I,J,H and K bands based on two fundamental pillars, namely omega Centauri and 47 Tucanae, have been obtained by using a large optical and near infrared photometric database. Our best estimates give M_I(TRGB)= -4.05 pm 0.12, M_J(TRGB)= -5.20 pm 0.16, M_H(TRGB)= -5.94 pm 0.18 and M_K(TRGB) = -6.04 pm 0.16 at [M/H]=-1.5 (omega Cen) and M_I(TRGB)= -3.91 pm 0.13, M_J(TRGB)= -5.47 pm 0.25, M_H(TRGB)= -6.35 pm 0.30 and M_K(TRGB)= -6.56 pm 0.20 at [M/H]=-0.6 (47 Tuc). With these new empirical calibrations we also provide robust relations of the TRGB magnitude in I, J, H and K bands as a function of the global metallicity ([M/H]). It has also been shown that our calibrations self-consistently provide a distance modulus of the Large Magellanic Cloud in good agreement with the standard value ((m-M)_0 = 18.50)).
arXiv commentA&A latex, 14 pages, 7 .ps figures (fig. 1 and fig. 3 provided in low resolution version). Accepted by Astronomy & Astrophysics Correction of a typographical error in Fig. 7; M_I vs [M/H] relation
References in corpus (35)
- Color Transformations for the 2MASS Second Incremental Data Release
- Abundances for Globular Cluster Giants: I. Homogeneous Metallicities for 24 Clusters
- Homogeneous Photometry for Star Clusters and Resolved Galaxies. II. Photometric Standard Stars
- VLT/UVES Abundances in Four Nearby Dwarf Spheroidal Galaxies: I. Nucleosynthesis and Abundance Ratios
- Distances, ages, and epoch of formation of globular clusters
- The giant, horizontal and asymptotic branches of galactic globular clusters. I. The catalog, photometric observables and features
- Distances and ages of NGC 6397, NGC 6752 and 47 Tuc
- New evidence for the complex struscture of the RGB of Omega Cen
- Red Giant Branch stars: the theoretical framework
- Deviations from the Local Hubble Flow. I. The Tip of the Red Giant Branch as a Distance Indicator
- A step toward the calibration of the RGB Tip as a Standard Candle
- A new IR-Array photometric survey of Galactic Globular Clusters: A detailed study of the RGB sequence as a step towards the global testing of stellar models
- The Draco and Ursa Minor dwarf spheroidals. A comparative study
- The Abundance Spread Among Giants and Subgiants in the Globular Cluster Omega Centauri
- Abundance Analysis of Turn-Off and Early Subgiant Stars in the Globular Cluster 47 Tuc (NGC 104)
- A new analysis of the Red Giant Branch "Tip" distance scale and the value of the Hubble constant
- A Digital Photometric Survey of the Magellanic Clouds: First Results From One Million Stars
- The White Dwarf Distance to the Globular Cluster 47 Tucanae and its Age
- High resolution spectroscopy of metal rich giants in omega Cen: first indication of SNe Ia enrichment
- Dust and Stellar Populations in the Large Magellanic Cloud
- The Resolved Stellar Populations in NGC 1705
- Chemical Abundances in Twelve Red Giants of the Large Magellanic Cloud from High-Resolution Infrared Spectroscopy
- A near-infrared spectroscopic screening of the red giant populations in omega Centauri
- The Stellar Populations of Pixels and Frames
- CCD Photometry of the Globular Cluster Omega Centauri. I. Metallicity of RR Lyrae Stars from Caby Photometry
- Tip of the Red Giant Branch Distances to NGC 4214, UGC 685, and UGC 5456
- Ultraviolet Properties of Primeval Galaxies: Theoretical Models from Stellar Population Synthesis
- Cluster AgeS Experiment. CCD photometry of SX Phoenicis variables in the globular cluster M 55
- The Tip of the Red Giant Branch Distance to the Large Magellanic Cloud
- Variations in Star Formation History and the Red Giant Branch Tip
- Background galaxies as reddening probes throughout the Magellanic Clouds
- Resolving the 47 Tucanae Distance Problem
- Automatic abundance analysis of high resolution spectra
- TNG Near-IR Photometry of five Galactic Globular Clusters
- Cluster AgeS Experiment (CASE): RR Lyrae stars from the globular cluster Omega Centauri as standard candles
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