no code implementations • 24 Feb 2021 • M. Tailo, A. P. Milone, E. P. Lagioia, F. D'Antona, S. Jang, E. Vesperini, A. F. Marino, P. Ventura, V. Caloi, M. Carlos, G. Cordoni, E. Dondoglio, A. Mohandasan, J. E. Nastasio, M. V. Legnardi
The mass losses inferred for the stellar populations with pristine chemical composition (called first-generation or 1G stars) tightly correlate with cluster metallicity.
Solar and Stellar Astrophysics Astrophysics of Galaxies
1 code implementation • 2 Nov 2011 • A. P. Milone, G. Piotto, L. R. Bedin, A. Aparicio, J. Anderson, A. Sarajedini, A. F. Marino, A. Moretti, M. B. Davies, B. Chaboyer, A. Dotter, M. Hempel, A. Marin-Franch, S. Majewski, N. E. Q. Paust, I. N. Reid, A. Rosenberg, M. Siegel
We studied the radial distribution of binary stars, and the distribution of stellar mass ratios.
Solar and Stellar Astrophysics
