Review
Open access
Aug 2026
The deepest color-magnitude diagrams for the benchmark open cluster NGC,2437 from Gaia and VVVX
Deep photometry of Galactic star clusters provides one of the most powerful tools for determining their physical properties. In particular, in low Galactic latitude regions that suffer from heavy extinction and crowding, it is essential to have accurate optical and near-IR photometry for benchmark clusters. NGC,2437 is...
T. Palma, M. Gómez, D. Minniti et al.
· Astronomy & Astrophysics · 0 citations