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researcher

E. Vesperini

173 papers hereh-index 415.9k citations249 works total

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

author position
  • sole author2
  • first author13
  • middle author102
  • last author36

Across the 153 of 173 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA108
  • astro-ph.SR51
  • astro-ph9
  • astro-ph.HE2
  • astro-ph.IM2
  • astro-ph.CO1
same name
  • E. Vesperini — 1 paper

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
19972026
most citedFormation and Dynamical Evolution of Multiple Stellar Generations in Globular Clusters

667 citations · 6.9k across the 171 of their papers we have counts for

collaborators
Showing 2020 · astro-ph.GAShow all

3 papers · 2 filters

astro-ph.GA2020★ 29 cited

Radial variation of the stellar mass functions in the globular clusters M15 and M30: clues of a non-standard IMF?

Mario Cadelano, Emanuele Dalessandro, Jeremy J. Webb +5

We exploit a combination of high-resolution Hubble Space Telescope and wide-field ESO-VLT observations to study the slope of the global mass function (alphaG) and its radial variat…

astro-ph.GA2020★ 6 cited

Substructure in the Globular Cluster Populations of the Virgo Cluster Elliptical Galaxies M84 and M86

Ryan A. Lambert, Katherine L. Rhode, Enrico Vesperini

We have carried out a search for substructure within the globular cluster systems of M84 (NGC 4374) and M86 (NGC 4406), two giant elliptical galaxies in the Virgo Cluster. We use w…

astro-ph.GA2020★ 29 cited

The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters. XX. Ages of single and multiple stellar populations in seven bulge globular clusters

R. A. P. Oliveira, S. O. Souza, L. O. Kerber +23

In the present work we analyzed seven globular clusters selected from their location in the Galactic bulge and with metallicity values in the range $-1.30\lesssim\rm{[Fe/H]}\lesssi…

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