most citedSurvey of multiple populations in globular clusters among very low-mass stars

28 citations · 101 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA20229 cited

The chemical compositions of multiple stellar populations in the globular cluster NGC 2808

M. Carlos, A. F. Marino, A. P. Milone +8

Pseudo two-colour diagrams or Chromosome maps (ChM) indicate that NGC 2808 host five different stellar populations. The existing ChMs have been derived by the Hubble Space Telescop…

astro-ph.GA202227 cited

Chromosome maps of Globular Clusters from wide-field ground-based photometry

S. Jang, A. P. Milone, M. V. Legnardi +10

Hubble Space Telescope (HST) photometry is providing an extensive analysis of globular clusters (GCs). In particular, the pseudo two-colour diagram dubbed 'chromosome map (ChM)' al…

astro-ph.GA2022

Constraining the original composition of the gas forming first-generation stars in globular clusters

M. V. Legnardi, A. P. Milone, L. Armillotta +13

Disentangling distinct stellar populations along the red-giant branches (RGBs) of Globular Clusters (GCs) is possible by using the pseudo two-color diagram dubbed chromosome map (C…

astro-ph.SR202228 cited

Survey of multiple populations in globular clusters among very low-mass stars

E. Dondoglio, A. P. Milone, A. Renzini +14

Recent work has shown that NIR Hubble Space Telescope (HST) photometry allows us to disentangle multiple populations (MPs) among M dwarfs of globular clusters (GCs) and investigate…

astro-ph.GA202113 cited

Integrated photometry of multiple stellar populations in Globular Clusters

S. Jang, A. P. Milone, E. P. Lagioia +8

Evidence that the multiple populations (MPs) are common properties of globular clusters (GCs) is accumulated over the past decades from clusters in the Milky Way and in its satelli…

astro-ph.SR202124 cited

Mass loss law for red giant stars in simple population globular clusters

M. Tailo, A. P. Milone, E. P. Lagioia +12

The amount of mass lost by stars during the red-giant branch (RGB) phase is one of the main parameters to understand and correctly model the late stages of stellar evolution. Never…