A Megacam Survey of Outer Halo Satellites. VI. The Spatially resolved Starformation History of the Carina Dwarf Spheroidal Galaxy*

We present the spatially resolved star-formation history (SFH) of the Carina dwarf spheroidal galaxy, obtained from deep, wide-field g and r imaging and a metallicity distribution from the literature. Our photometry covers similar to 2 deg(2), reaching up to similar to 10 times the half-light radius of Carina with a completeness higher than 50% at g similar to 24.5, more than one magnitude fainter than the oldest turnoff. This is the first time a combination of depth and coverage of this quality has been used to derive the SFH of Carina, enabling us to trace its different populations with unprecedented accuracy. We find that Carina's SFH consists of two episodes well separated by a star-formation temporal gap. These episodes occurred at old (>10 Gyr) and intermediate (2-8 Gyr) ages. Our measurements show that the old episode comprises the majority of the population, accounting for 54 +/- 5% of the stellar mass within 1.3 times the King tidal radius, while the total stellar mass derived for Carina is 1.60 +/- 0.09 x 10(6) M-circle dot, and the stellar mass-to-light ratio is 1.8 +/- 0.2. The SFH derived is consistent with no recent star formation, which hints that the observed blue plume is due to blue stragglers. We conclude that the SFH of Carina evolved independently of the tidal field of the Milky Way, since the frequency and duration of its star-formation events do not correlate with its orbital parameters. This result is supported by the age-metallicity relation observed in Carina. and the gradients calculated indicating that outer regions are older and more metal-poorCONICYT Anillo project ACT-1122 CONICYT BASAL PFB-06 FONDECYT project 1120013 National Science Foundation AST-0908752 Alfred P. Sloan Foundation NSF AST-1313422 AST-1413600 AST-1518308 FONDECYT 315057