activity
19992023
most citedGravity modes as a way to distinguish between hydrogen- and helium-burning red giant stars

612 citations · 6k across the 122 of their papers we have counts for

collaborators

123 papers

astro-ph.GA2023

A deep dive into the Type II Globular Cluster NGC 1851

E. Dondoglio, A. P. Milone, A. F. Marino +13

About one-fifth of the Galactic globular clusters (GCs), dubbed Type II GCs, host distinct stellar populations with different heavy elements abundances. NGC 1851 is one of the most…

astro-ph.SR2023★ 5 cited

Unravelling the Period Gap using LAMOST Chromospheric Activity Indices

Deepak Chahal, Devika Kamath, Richard de Grijs +2

In our recent catalogue of BY Draconis (BY Dra) variables based on Zwicky Transient Facility data, we found traces of a period gap in the period-colour diagram. We combined our BY…

astro-ph.SR2023★ 13 cited

Hubble Space Telescope survey of Magellanic Cloud star clusters. UV-dim stars in young clusters

A. P. Milone, G. Cordoni, A. F. Marino +11

Young and intermediate-age star clusters of both Magellanic Clouds exhibit complex color-magnitude diagrams. In addition to the extended main-sequence turn-offs (eMSTOs), commonly…

astro-ph.SR2023★ 2 cited

An insight into Capella (alpha Aurigae): from the extent of core overshoot to its evolutionary history

E. Marini, C. Ventura, M. Tailo +3

The binary star alpha Aurigae (otherwise known as Capella) is extremely important to understand the core hydrogen and helium burning phases of the stars, as the primary star is lik…

astro-ph.SR2023★ 18 cited

On the role of dust and mass loss in the extended main sequence turnoff of star clusters: the case of NGC 1783

F. D'Antona, F. Dell'Agli, M. Tailo +6

The Color Magnitude Diagram (CMD) morphology of the "extended" main sequence turnoff (eMSTO) and upper main sequence (MS) of the intermediate age ( Gyr) Large Magellani…

astro-ph.SR2023★ 13 cited

A study of carbon-rich post-AGB stars in the Milky Way to understand the production of carbonaceous dust from evolved stars

Silvia Tosi, Devika Kamath, Flavia Dell'Agli +5

The goal of this study is to reconstruct the evolution and the dust formation processes during the final AGB phases of a sample of carbon-rich, post-AGB Galactic stars, with partic…