ON THE ABSOLUTE AGE OF THE METAL-RICH GLOBULAR M71 (NGC 6838). I. OPTICAL PHOTOMETRY

We investigated the absolute age of the Galactic globular cluster M71 (NGC 6838) using optical ground-based images ( u ′ , g ′ , r ′ , i ′ , z ′ ?> ) collected with the MegaCam camera at the Canada–France–Hawaii Telescope (CFHT). We performed a robust selection of field and cluster stars by applying a new method based on the 3D ( r ′ , u ′ − g ′ , g ′ − r ′ ?> ) color–color–magnitude diagram. A comparison between the color–magnitude diagram (CMD) of the candidate cluster stars and a new set of isochrones at the locus of the main sequence turn-off (MSTO) suggests an absolute age of 12 ± 2 Gyr. The absolute age was also estimated using the difference in magnitude between the MSTO and the so-called main sequence knee, a well-defined bending occurring in the lower main sequence. This feature was originally detected in the near-infrared bands and explained as a consequence of an opacity mechanism (collisionally induced absorption of molecular hydrogen) in the atmosphere of cool low-mass stars. The same feature was also detected in the r′, u ′ − g ′ ?> , and in the r ′ , g ′ − r ′ ?> CMD, thus supporting previous theoretical predictions by Borysow et al. The key advantage in using the Δ TO Knee ?> as an age diagnostic is that it is independent of uncertainties affecting the distance, the reddening, and the photometric zero point. We found an absolute age of 12 ± 1 Gyr that agrees, within the errors, with similar age estimates, but the uncertainty is on average a factor of two smaller. We also found that the Δ TO Knee ?> is more sensitive to the metallicity than the MSTO, but the dependence vanishes when using the difference in color between the MSK and the MSTO.

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