activity
20162023
most citedTarget Selection for the SDSS-IV APOGEE-2 Survey

293 citations · 718 across the 16 of their papers we have counts for

collaborators

29 papers

astro-ph.SR2025

Mass loss along the red giant branch of the intermediate stellar populations in NGC6752 and NGC2808

M. Tailo, A. P. Milone, A. F. Marino +15

The morphology of the Horizontal Branch (HB) in Globular Clusters (GC) is among the early evidences that they contain multiple populations of stars. Indeed, the location of each st…

astro-ph.SR20254 cited

Planetary Nebulae of the Large Magellanic Cloud II: the connection with the progenitors' properties

P. Ventura, S. Tosi, D. A. García-Hernández +6

The study of planetary nebulae (PNe) offers the opportunity of evaluating the efficiency of the dust production mechanism during the very late asymptotic giant branch (AGB) phases.…

astro-ph.SR2023

GN-z11: witnessing the formation of second generation stars and an accreting massive black hole in a massive star cluster

F. D'Antona, E. Vesperini, F. Calura +7

We explore the possibility that the N-rich young proto-galaxy GN-z11 recently observed at z=10.6 by the James Webb Space Telescope is the result of the formation of second generati…

astro-ph.GA2022

Carbon Abundances in Compact Galactic Planetary Nebulae: An Ultraviolet spectroscopic study with the Space Telescope Imaging Spectrograph (STIS)

Letizia Stanghellini, Rafia Bushra, Richard A. Shaw +3

We surveyed a sample of compact Galactic planetary nebulae (PNe) with the Space Telescope Imaging Spectrograph on the Hubble Space Telescope (HST/STIS) to determine their gas-phase…

astro-ph.SR202213 cited

HST observations of the globular cluster NGC 6402 (M14) and its peculiar multiple populations

Francesca D'Antona, Antonino P. Milone, Christian I. Johnson +6

We present Hubble Space Telescope (HST) photometric results for NGC 6402, a highly reddened very luminous Galactic globular cluster (GC). Recent spectroscopic observations of its r…

astro-ph.SR2021

Gas and dust from extremely metal-poor AGB stars

P. Ventura, F. Dell'Agli, D. Romano +8

We study the evolution of extremely metal-poor AGB stars, with metallicities down to [Fe/H]=-5, to understand the main evolutionary properties, the efficiency of the processes able…