no code implementations • 8 Feb 2021 • K. Peña Ramírez, C. González-Fernández, A. -N. Chené, S. Ramírez Alegría
Open clusters are central elements of our understanding of the Galactic disk evolution, as an accurate determination of their parameters leads to an unbiased picture of our Galaxy's structure.
Astrophysics of Galaxies Solar and Stellar Astrophysics
no code implementations • 5 Oct 2020 • E. R. Garro, D. Minniti, M. Gómez, J. Alonso-García, R. H. Barbá, B. Barbuy, J. J. Clariá, A. N. Chené, B. Dias, M. Hempel, V. D. Ivanov, P. W. Lucas, D. Majaess, F. Mauro, C. Moni Bidin, T. Palma, J. B. Pullen, R. K. Saito, L. Smith, F. Surot, S. Ramírez Alegría, M. Rejkuba, V. Ripepi
Milky Way globular clusters (MW GCs) are difficult to identify at low Galactic latitudes because of high differential extinction and heavy star crowding.
Astrophysics of Galaxies Solar and Stellar Astrophysics
