no code implementations • 26 Jan 2021 • Matteo Correnti, Paul Goudfrooij, Andrea Bellini, Leo Girardi
We present the analysis of the colour-magnitude diagram (CMD) morphology of the ~ 800 Myr old star cluster NGC1831 in the Large Magellanic Cloud, exploiting deep, high-resolution photometry obtained using the Wide Field Camera 3 onboard the Hubble Space Telescope.
Astrophysics of Galaxies Solar and Stellar Astrophysics
