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researcher

S. Tosi

3 papers here

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

author position
  • first author2
  • middle author1

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR3
ORCID 0009-0000-7695-9304
same name
  • S. Tosi — 256 papers
  • S. Tosi — 45 papers, h 115
  • S. Tosi — 27 papers, h 0
  • S. Tosi — 6 papers
  • S. Tosi — 4 papers, h 42
  • S. Tosi — 3 papers

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

most citedUnderstanding dust production and mass loss on the AGB phase using post-AGB stars in the Magellanic Clouds

15 citations · 28 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.SR2023

Dust from evolved stars: a pilot analysis of the AGB to PN transition

F. Dell'Agli, S. Tosi, D. Kamath +5

We present a novel approach to address dust production by low- and intermediate-mass stars. We study the asymptotic giant branch (AGB) phase, during which the formation of dust tak…

astro-ph.SR2023★ 13 cited

A study of carbon-rich post-AGB stars in the Milky Way to understand the production of carbonaceous dust from evolved stars

Silvia Tosi, Devika Kamath, Flavia Dell'Agli +5

The goal of this study is to reconstruct the evolution and the dust formation processes during the final AGB phases of a sample of carbon-rich, post-AGB Galactic stars, with partic…

astro-ph.SR2022★ 15 cited

Understanding dust production and mass loss on the AGB phase using post-AGB stars in the Magellanic Clouds

Silvia Tosi, Flavia Dell'Agli, Devika Kamath +3

Aims: We aim to understand the variation of the surface chemistry that occurs during the AGB phase by analysing results from observations of single post-AGB stars in the Magellanic…

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