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S. Pezzuto

91 papers hereh-index 479.8k citations223 works total

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

author position
  • first author2
  • middle author58
  • last author3

Across the 63 of 91 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA66
  • astro-ph.SR10
  • astro-ph.IM8
  • astro-ph6
  • astro-ph.EP1
same name
  • S. Pezzuto — 12 papers
  • S. Pezzuto — 11 papers, h 2
  • S. Pezzuto — 1 paper, h 1
  • S. Pezzuto — 1 paper, h 1

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
19992025
most citedFrom filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the Herschel Gould Belt survey

1.5k citations · 9.9k across the 91 of their papers we have counts for

collaborators
Showing 2023Show all

3 papers · 1 filter

astro-ph.IM2023★ 4 cited

A new tool to derive simultaneously exponent and extremes of power-law distributions

S. Pezzuto, A. Coletta, R. S. Klessen +6

Many experimental quantities show a power-law distribution p(x)∝x−α. In astrophysics, examples are: size distribution of dust grains or luminosity function of galaxies.…

astro-ph.GA2023★ 14 cited

A panoptic view of the Taurus molecular cloud I. The cloud dynamics revealed by gas emission and 3D dust

J. D. Soler, C. Zucker, J. E. G. Peek +14

We present a study of the three-dimensional (3D) distribution of interstellar dust derived from stellar extinction observations toward the Taurus molecular cloud (MC) and its relat…

astro-ph.GA2023★ 35 cited

The SQUALO project (Star formation in QUiescent And Luminous Objects) I: clump-fed accretion mechanism in high-mass star-forming objects

A. Traficante, B. M. Jones, A. Avison +10

The formation mechanism of the most massive stars is far from completely understood. It is still unclear if the formation is core-fed or clump-fed, i.e. if the process is an extens…

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