Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 454, Issue 2, Pages 1509-1516Publisher
OXFORD UNIV PRESS
DOI: 10.1093/mnras/stv2014
Keywords
stars: variables: RR Lyrae; galaxies: evolution; galaxies: individual: Sculptor dSph; Local Group; galaxies: stellar content
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Funding
- Spanish Ministry of Economy and Competitiveness (MINECO) [AYA2014-56795]
- National Science Centre, Poland [MAESTRO 2014/14/A/ST9/00121]
- Futuro in Ricerca [RBFR13J716]
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We identified and characterized the largest (536) RR Lyrae (RRL) sample in a Milky Way dSph satellite (Sculptor) based on optical photometry data collected over similar to 24 years. The RRLs display a spread in V-magnitude (similar to 0.35 mag) which appears larger than photometric errors and the horizontal branch (HB) luminosity evolution of a mono-metallic population. Using several calibrations of two different reddening free and metal independent period-Wesenheit relations we provide a new distance estimate mu = 19.62 mag (sigma(mu) = 0.04 mag) that agrees well with literature estimates. We constrained the metallicity distribution of the old population, using the M-I period-luminosity relation, and we found that it ranges from -2.3 to -1.5 dex. The current estimate is narrower than suggested by low and intermediate spectroscopy of RGBs (Delta [Fe/H]<= 1.5). We also investigated the HB morphology as a function of the galactocentric distance. The HB in the innermost regions is dominated by red HB stars and by RRLs, consistent with a more metal-rich population, while in the outermost regions it is dominated by blue HB stars and RRLs typical of a metal-poor population. Our results suggest that fast chemical evolution occurred in Sculptor, and that the radial gradients were in place at an early epoch.
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