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researcher

A. Ferrara

43 papers hereh-index 211.5k citations62 works total

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

author position
  • first author2
  • middle author34
  • last author3

Across the 39 of 43 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA32
  • astro-ph.CO6
  • astro-ph4
  • astro-ph.HE1
same name
  • A. Ferrara — 257 papers, h 68
  • A. Ferrara — 32 papers, h 18
  • A. Ferrara — 28 papers, h 7
  • A. Ferrara — 20 papers, h 7
  • A. Ferrara — 14 papers, h 7
  • A. Ferrara — 11 papers, h 5

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
20052025
most citedFragmentation of star-forming clouds enriched with the first dust

302 citations · 2.4k across the 42 of their papers we have counts for

collaborators
Showing astro-phShow all

4 papers · 1 filter

astro-ph2008★ 4 cited

Effects of dark matter annihilation on the first stars

F. Iocco, A. Bressan, E. Ripamonti +3

We study the evolution of the first stars in the universe (Population III) from the early pre-Main Sequence until the end of helium burning in the presence of WIMP dark matter anni…

astro-ph2008★ 78 cited

Dark matter annihilation effects on the first stars

F. Iocco, A. Bressan, E. Ripamonti +3

We study the effects of WIMP dark matter (DM) on the collapse and evolution of the first stars in the Universe. Using a stellar evolution code, we follow the pre-Main Sequence (MS)…

astro-ph2006★ 302 cited

Fragmentation of star-forming clouds enriched with the first dust

Raffaella Schneider, Kazuyuki Omukai, Akio Inoue +1

The thermal and fragmentation properties of star-forming clouds have important consequences on the corresponding characteristic stellar mass. The initial composition of the gas wit…

astro-ph2005★ 101 cited

Constraints on the IMF of the first stars

R. Schneider, R. Salvaterra, A. Ferrara +1

Motivated by theoretical predictions that first stars were predominantly very massive, we investigate the physics of the transition from an early epoch dominated by massive Pop III…

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