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S. Larsen

19 papers hereh-index 253.1k citations88 works total

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

author position
  • sole author7
  • middle author5
  • last author3

Across the 15 of 19 papers where every author was matched, so the position is known.

fields
  • astro-ph17
  • astro-ph.CO2
same name
  • S. Larsen — 20 papers, h 33
  • S. Larsen — 6 papers, h 8
  • S. Larsen — 1 paper, h 2

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
20012011
most citedACS imaging of star clusters in M51. I. Identification and radius distribution

99 citations · 199 across the 11 of their papers we have counts for

collaborators
Showing 2006Show all

4 papers · 1 filter

astro-ph2006

Variation of the cluster luminosity function across the disk of M51

M. R. Haas, M. Gieles, R. A. Scheepmaker +3

We study the luminosity function (LF) of the star clusters in M51. Comparing the observed LF with the LF resulting from artificial cluster populations suggests that there exists an…

astro-ph2006★ 14 cited

Planetary Nebula Candidates in Extragalactic Young Star Clusters

S. S. Larsen, T. Richtler

During an analysis of optical spectra of 80 young star clusters in several nearby spiral galaxies, [O III] and [N II] emission lines were noted in some cases. Three of these emissi…

astro-ph2006★ 1 cited

Young Massive Clusters - Formation Efficiencies and (Initial) Mass Functions

Soeren S. Larsen

Globular clusters are often assumed to be good tracers of major star formation episodes in their host galaxies. While observations over the past 2 decades have confirmed the presen…

astro-ph2006

The luminosity function of young star clusters: implications for the maximum mass and luminosity of clusters

Mark Gieles, Soeren Larsen, Nate Bastian +1

We introduce a method to relate a possible truncation of the star cluster mass function at the high mass end to the shape of the cluster luminosity function (LF). We compare the ob…

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