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S. Bontemps

100 papers hereh-index 405.4k citations165 works total

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

author position
  • first author2
  • middle author71
  • last author2

Across the 75 of 100 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA75
  • astro-ph.SR18
  • astro-ph5
  • astro-ph.IM2
same name
  • S. Bontemps — 88 papers, h 52
  • S. Bontemps — 7 papers
  • S. Bontemps — 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
20002025
most citedFrom filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the Herschel Gould Belt survey

1.5k citations · 9.6k across the 100 of their papers we have counts for

collaborators
Showing 2018 · astro-ph.GAShow all

3 papers · 2 filters

astro-ph.GA2018★ 167 cited

Characterizing young protostellar disks with the CALYPSO IRAM-PdBI survey: large Class 0 disks are rare

A. J. Maury, Ph. André, L. Testi +15

Understanding the formation mechanisms of protoplanetary disks and multiple systems, and their pristine properties, is a key question for modern astrophysics. The properties of the…

astro-ph.GA2018★ 52 cited

The search for high-mass protostars with ALMA revealed up to kilo-parsec scales (SPARKS): I. Indication for a centrifugal barrier in the environment of a single high-mass envelope

T. Csengeri, S. Bontemps, F. Wyrowski +11

The formation of the most massive O-type stars is poorly understood. We present a case study of a young massive clump from the ATLASGAL survey, G328.2551-0.5321. It exhibits a bolo…

astro-ph.GA2018★ 140 cited

The unexpectedly large proportion of high-mass star-forming cores in a Galactic mini-starburst

F. Motte, T. Nony, F. Louvet +14

Understanding the processes that determine the stellar Initial Mass Function (IMF) is a critical unsolved problem, with profound implications for many areas of astrophysics. In mol…

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