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C. Weidner

35 papers hereh-index 253k citations52 works total

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

author position
  • first author20
  • middle author5
  • last author4

Across the 29 of 35 papers where every author was matched, so the position is known.

fields
  • astro-ph16
  • astro-ph.GA7
  • astro-ph.CO6
  • astro-ph.SR5
  • astro-ph.EP1
same name
  • C. Weidner — 22 papers, h 10
  • C. Weidner — 8 papers, h 4
  • C. Weidner — 5 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
20032015
most citedGalactic-Field IMFs of Massive Stars

525 citations · 3.6k across the 35 of their papers we have counts for

collaborators
Showing 2007 · astro-phShow all

4 papers · 2 filters

astro-ph2007

A Search for EHB Pulsators in the Globular Cluster NGC 6752

M. Catelan, G. E. Prieto, M. Zoccali +8

We describe the status of a project whose main goal is to detect variability along the extreme horizontal branch of the globular cluster NGC 6752. Based on Magellan 6.5m data, prel…

astro-ph2007★ 1 cited

Converting Halpha luminosities into SFRs

Jan Pflamm-Altenburg, Carsten Weidner, Pavel Kroupa

Star-formation rates (SFRs) of galaxies are commonly calculated by converting the measured Halpha luminosities (L_Halpha) into current SFRs. This conversion is based on a constant…

astro-ph2007★ 138 cited

Converting Hα Luminosities into Star Formation Rates

Jan Pflamm-Altenburg, Carsten Weidner, Pavel Kroupa

The recent finding that the IGIMF (integrated galaxial initial stellar mass function) composed of all newly formed stars in all young star clusters has, in dependence of the SFR, a…

astro-ph2007★ 38 cited

On the infant weight loss of low- to intermediate-mass star clusters

C. Weidner, P. Kroupa, D. E. A. Nuernberger +1

Star clusters are born in a highly compact configuration, typically with radii of less than about 1 pc roughly independently of mass. Since the star-formation efficiency is less th…

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