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S. Ortolani

61 papers hereh-index 4912.1k citations528 works total

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

author position
  • first author4
  • middle author35
  • last author11

Across the 50 of 61 papers where every author was matched, so the position is known.

fields
  • astro-ph20
  • astro-ph.GA17
  • astro-ph.SR16
  • astro-ph.IM4
  • astro-ph.EP2
  • physics.geo-ph1
same name
  • S. Ortolani — 63 papers, h 27
  • S. Ortolani — 9 papers, h 7
  • S. Ortolani — 7 papers, h 8
  • S. Ortolani — 4 papers
  • S. Ortolani — 1 paper, h 0

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
19962023
most citedThe Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters. I. Overview of the Project and Detection of Multiple Stellar Populations

509 citations · 4.3k across the 61 of their papers we have counts for

collaborators
Showing 2003 · astro-phShow all

3 papers · 2 filters

astro-ph2003★ 79 cited

Gemini-Phoenix infrared high-resolution abundance analysis of five giants in the bulge globular cluster NGC 6553

J. Melendez, B. Barbuy, E. Bica +4

A detailed abundance analysis of 5 giants of the metal-rich bulge globular cluster NGC 6553 was carried out using high resolution infrared spectra in the H band, obtained at the Ge…

astro-ph2003★ 33 cited

NTT infrared imaging of star cluster candidates towards the central parts of the Galaxy

C. M. Dutra, S. Ortolani, E. Bica +3

We address the issue whether the central parts of the Galaxy harbour young clusters other than Arches, Quintuplet and the Nuclear Young Cluster. A large sample of centrally project…

astro-ph2003★ 20 cited

The Wilson--Bappu Effect: a tool to determine stellar distances

Giancarlo Pace, Luca Pasquini, Sergio Ortolani

Wilson and Bappu (1957) have shown the existence of a remarkable correlation between the width of the emission in the core of the K line of Ca II and the absolute visual magnitude…

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