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researcher

G. Santoro

5 papers hereh-index 201.9k citations89 works total

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

author position
  • first author2
  • middle author3

Across the 5 of 5 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA3
  • astro-ph.IM2
same name
  • G. Santoro — 67 papers, h 36
  • G. Santoro — 40 papers, h 16
  • G. Santoro — 1 paper, h 20
  • G. Santoro — 1 paper, h 2
  • G. Santoro — 1 paper, h 3
  • G. Santoro — 1 paper, h 4

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
20172021
most citedThe chemistry of cosmic dust analogues from C, C2​, and C2​H2​ in C-rich circumstellar envelopes

45 citations · 95 across the 5 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

3 papers · 1 filter

astro-ph.GA2021★ 11 cited

Structure, stability and optical absorption spectra of small Tin​Cx​ clusters: a first-principles approach

Sergio Gámez-Valenzuela, Julio A. Alonso, Gonzalo Santoro +1

Titanium-carbide molecular clusters are thought to form in the circumstellar envelopes (CSEs) of carbon-rich Asymptotic Giant Branch stars (AGBs) but, to date, their detection has…

astro-ph.GA2020★ 18 cited

Silicon and hydrogen chemistry under laboratory conditions mimicking the atmosphere of evolved stars

Mario Accolla, Gonzalo Santoro, Pablo Merino +10

Silicon is present in interstellar dust grains, meteorites and asteroids, and to date thirteen silicon-bearing molecules have been detected in the gas-phase towards late-type stars…

astro-ph.GA2020★ 45 cited

The chemistry of cosmic dust analogues from C, C2​, and C2​H2​ in C-rich circumstellar envelopes

Gonzalo Santoro, Lidia Martínez, Koen Lauwaet +13

Interstellar carbonaceous dust is mainly formed in the innermost regions of circumstellar envelopes around carbon-rich asymptotic giant branch (AGB) stars. In these highly chemical…

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