activity
19982026
most citedAbundance Gradients and the Formation of the Milky Way

688 citations · 4.9k across the 96 of their papers we have counts for

collaborators

98 papers

astro-ph.GA2026

CRIMSONS: An Online Tool for Modeling Chemical Enrichment with Stochastic IMF Sampling

Martina Rossi, Lapo Querci, Stefano Ciabattini +14

Chemical enrichment is a universal process shaped by several interconnected factors, including stellar feedback, the nature of chemical polluters, and the underlying distribution o…

astro-ph.GA2025

Cosmic Threads: Interlinking the Stellar Initial Mass Function from Star-Birth to Galaxies

Tereza Jerabkova, Donatella Romano, Pavel Kroupa +19

The stellar initial mass function (sIMF) describes the distribution of stellar masses formed in a single star formation event in a molecular cloud clump. It is fundamental to astro…

astro-ph.GA2023★ 5 cited

A Systematic Observational Study on Galactic Interstellar Ratio 18O/17O. II. C18O and C17O J=2-1 Data Analysis

Y. P. Zou, J. S. Zhang, C. Henkel +7

To investigate the relative amount of ejecta from high-mass versus intermediate-mass stars and to trace the chemical evolution of the Galaxy, we have performed with the IRAM 30m an…

astro-ph.GA2023

The chemical DNA of the Magellanic Clouds --II. High-resolution spectroscopy of the SMC globular clusters NGC 121, NGC 339 and NGC 419

A. Mucciarelli, A. Minelli, C. Lardo +5

The Small Magellanic Cloud (SMC) is the host of a rich system of globular clusters (GCs) that span a wide age range. The chemical composition of the SMC clusters is still poorly un…

astro-ph.GA2023★ 18 cited

Modeling the chemical enrichment history of the Bulge Fossil Fragment Terzan 5

Donatella Romano, Francesco R. Ferraro, Livia Origlia +9

Terzan 5 is a heavily obscured stellar system located in the inner Galaxy. It has been postulated to be a stellar relic, a Bulge Fossil Fragment witnessing the complex history of t…

astro-ph.GA2023★ 4 cited

OO abundance ratio toward a sample of massive star forming regions with parallax distances

Chao Ou, Junzhi Wang, Siqi Zheng +3

The OO abundance ratio is, in principle, a powerful tool to estimate the relative contributions of massive stars and low- to intermediate-mass stars to the chemical…