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Extinction in the Large Magellanic Cloud Bar around NGC1854, NGC1856, and NGC1858
Guido De Marchi, Nino Panagia, Antonino P. Milone
We report on the extinction properties in the fields around the clusters NGC 1854, NGC 1856, and NGC 1858 in the bar of the Large Magellanic Cloud. The colour-magnitude diagrams of…
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…
Spectroscopy and photometry of the least-massive Type-II globular clusters: NGC1261 AND NGC6934
A. F. Marino, A. P. Milone, A. Renzini +10
Recent work has revealed two classes of Globular Clusters (GCs), dubbed Type-I and Type-II. Type-II GCs are characterized by a blue- and a red- red giant branch composed of stars w…
A stringent upper limit on Be star fractions produced by binary interaction
B. Hastings, N. Langer, C. Wang +2
Context. Binary evolution can result in fast-rotating stars, predicted to be observable as Be stars, through accretion of angular momentum during mass-transfer phases. Despite nume…
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…
Multiple stellar populations in Asymptotic Giant Branch stars of Galactic Globular Clusters
E. P. Lagioia, A. P. Milone, A. F. Marino +8
Multiple stellar populations (MPs) are a distinct characteristic of Globular Clusters (GCs). Their general properties have been widely studied among main sequence, red giant branch…