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researcher

C. Chiosi

89 papers hereh-index 419.1k citations361 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author3
  • middle author43
  • last author36

Across the 82 of 89 papers where every author was matched, so the position is known.

fields
  • astro-ph49
  • astro-ph.GA25
  • astro-ph.CO7
  • astro-ph.SR7
  • astro-ph.IM1
same name
  • C. Chiosi — 7 papers

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
19952026
most citedEvolutionary tracks and isochrones for low- and intermediate-mass stars: from 0.15 to 7 M_sun, and from Z=0.0004 to 0.03

2.6k citations · 5.9k across the 89 of their papers we have counts for

collaborators
Showing 2001Show all

4 papers · 1 filter

astro-ph2001

A chemical evolution model for galaxy clusters

L. Portinari, A. Moretti, C. Chiosi

We develop a toy-model for the chemical evolution of the intracluster medium, polluted by the galactic winds from elliptical galaxies. The model follows the "galaxy formation histo…

astro-ph2001

Chemical Evolution of Clusters of Galaxies

L. Portinari, A. Moretti, C. Chiosi

The high metallicity of the intra-cluster medium (ICM) is generally interpreted on the base of the galactic wind scenario for elliptical galaxies. In this framework, we develop a t…

astro-ph2001★ 40 cited

Dwarf Elliptical Galaxies: Structure, Star Formation, and Color-Magnitude Diagrams

G. Carraro, C. Chiosi, L. Girardi +1

The aim of this paper is to cast light on the formation and evolution of elliptical galaxies by means of N-body/hydro-dynamical simulations that include star formation, feed-back a…

astro-ph2001★ 226 cited

Zero-metallicity stars I. Evolution at constant mass

Paola Marigo, Leo Girardi, Cesare Chiosi +1

We present extensive evolutionary models of stars with initial zero-metallicity, covering a large range of initial masses (i.e. 0.7 <= M <= 100 Msun). Calculations are carried out…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.