activity
20012026
most citedGRB 090423 at a redshift of z~8.1

498 citations · 1.7k across the 67 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

15 papers · 1 filter

astro-ph.GA2026

The internal kinematics and chemistry of 20 Milky Way strings

C. Boeche, A. Vallenari, J. Alonso-Santiago +8

Context: the recent discovery of filamentary stellar structures in the Milky Way disk raises the question of their formation in the context of the Galaxy evolution. Aims: in this w…

astro-ph.GA2026

Milky-Way-like stars in a galaxy core 8 billion years ago revealed by gravitational lensing

Quirino D'Amato, Filippo Mannucci, Alessandro Sonnenfeld +40

The assembly of stellar-dominated cores in elliptical galaxies is key to understanding how cosmic structures evolved. Gravitational lensing offers unique insights into the nature o…

astro-ph.GA2025

Stellar Population Astrophysics (SPA) with the TNG 23 IR elemental abundances of 114 giant stars in 41 Open Clusters

Shilpa Bijavara Seshashayana, Henrik Jönsson, Valentina D'Orazi +4

Open clusters have been extensively used as tracers of Galactic chemical evolution, as their constituent stars possess shared characteristics, including age, Galactocentric radius,…

astro-ph.GA2025

Low-Eddington ratio, changing-look active galactic nuclei: the case of NGC 4614

Elisabeta Lusso, Lapo Casetti, Marco Romoli +27

Active galactic nuclei (AGN) are known to be variable sources across the entire electromagnetic spectrum, in particular at optical/ultraviolet and X-ray energies. Over the past dec…

astro-ph.GA2024★ 6 cited

The Radcliffe Wave as traced by young open clusters: Stellar parameters, activity indicators, and abundances of solar-type members of eight young clusters

J. Alonso-Santiago, A. Frasca, A. Bragaglia +7

The Radcliffe Wave has only recently been recognised as a about 3 kpc long coherent gas structure encompassing most of the star forming regions in the solar vicinity. Since its dis…

astro-ph.GA2024★ 6 cited

Exploring fluorine chemical evolution in the Galactic disk: the open cluster perspective

Shilpa Bijavara Seshashayana, Henrik Jönsson, Valentina D'Orazi +6

Open clusters are ideal tools for tracing the abundances of different elements because their stars are expected to have the same age, distance, and metallicity. Therefore, they ser…