activity
20192025
most citedA Kilonova Following a Long-Duration Gamma-Ray Burst at 350 Mpc

356 citations · 436 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2025

A study of Andromeda to improve our knowledge on the evolution and dust production by AGB stars

Claudio Gavetti, Paolo Ventura, Flavia Dell'Agli +4

We study the AGB population of the galaxy M31, based on available HST and Spitzer data, to characterize the individual sources in terms of mass, metallicity and formation epoch of…

astro-ph.HE2023★ 16 cited

The spectra of IceCube Neutrino (SIN) candidate sources -- III. Optical spectroscopy and source characterization of the full sample

Simona Paiano, Renato Falomo, Aldo Treves +5

A correlation between astrophysical high-energy neutrinos and blazars has been suggested by various authors. In particular, a likely association between IceCube events and intermed…

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…

astro-ph.SR2023★ 13 cited

The intense production of silicates during the final AGB phases of intermediate mass stars

E. Marini, F. Dell'Agli, D. Kamath +7

The formation of silicates in circumstellar envelopes of stars evolving through the AGB is still debated given the uncertainties affecting stellar evolution modelling, the descript…

astro-ph.SR2022★ 9 cited

A study of oxygen-rich post-AGB stars in the Milky Way to understand the production of silicates from evolved stars

F. Dell'Agli, S. Tosi, D. Kamath +4

The study of post asymptotic giant branch (post-AGB) stars is a valuable tool to study still poorly known aspects of the evolution of the stars through the AGB. This is due to the…

astro-ph.SR2022★ 15 cited

Understanding dust production and mass loss on the AGB phase using post-AGB stars in the Magellanic Clouds

Silvia Tosi, Flavia Dell'Agli, Devika Kamath +3

Aims: We aim to understand the variation of the surface chemistry that occurs during the AGB phase by analysing results from observations of single post-AGB stars in the Magellanic…