GeMS MCAO observations of the Galactic globular cluster NGC 2808: the absolute age

TL;DR

This study accurately determines the absolute age of the globular cluster NGC 2808 using deep infrared and optical data, achieving unprecedented precision and providing insights into Galactic formation history.

Contribution

It introduces a new age estimation method based on the Main Sequence Knee feature, reducing systematic uncertainties compared to classical techniques.

Findings

NGC 2808's age is 10.9±0.7 Gyr.

The method reduces age uncertainty by a factor of three.

NGC 2808 is slightly younger than similar metallicity clusters.

Abstract

Globular clusters are the oldest stellar systems in the Milky Way and probe the early epoch of the Galaxy formation. However, the uncertainties on their absolute age are still too large to soundly constrain how the Galactic structures have assembled. The aim of this work is to obtain an accurate estimate of the absolute age of the globular cluster NGC 2808 using deep IR data obtained with the multi conjugate adaptive optics system operating at the Gemini South telescope (GeMS). This exquisite photometry, combined with that obtained in V and I bands with HST, allowed us the detection of the faint Main Sequence Knee feature in NGC 2808 colour magnitude diagram. The difference between this point and the main sequence turn off is a good age estimator and provides ages with unprecedented accuracy. We found that NGC 2808 has an age of t=10.9\pm0.7 (intrinsic) \pm0.45 (metallicity term) Gyr. A possible contamination by He-enhanced population could make the cluster up to 0.25 Gyr older. Although this age estimate agrees with the age coming from the classical turn off method (t=11.0 Gyr), its uncertainty is a factor ~3 better, since it avoids systematics in reddening, distance assumptions and photometric zero points determination. The final absolute age indicates that NGC 2808 is slightly younger than other Galactic globular clusters with similar metallicity.