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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 2004 · astro-phShow all

4 papers · 2 filters

astro-ph2004

IMF variations and their implications for Supernovae numbers

C. Weidner, P. Kroupa

The stellar initial mass function (IMF) integrated over an entire galaxy is an integral over all separate star-formation events. Since most stars form in star clusters with differe…

astro-ph2004★ 12 cited

Variation of the IMF

Pavel Kroupa, Carsten Weidner

(abridged) The {stellar IMF} has been found to be essentially invariant. While some apparent differences are seen, the uncertainties inherent to this game do not allow a firm concl…

astro-ph2004

Monte-Carlo experiments on star-cluster induced integrated-galaxy IMF variations

Carsten Weidner, Pavel Kroupa

As most if not all stars are born in stellar clusters the shape of the mass function of the field stars is not only determined by the initial mass function of stars (IMF) but also…

astro-ph2004★ 202 cited

Implications for the formation of star clusters from extra-galactic star-formation rates

C. Weidner, P. Kroupa, S. S. Larsen

Observations indicate that young massive star clusters in spiral and dwarf galaxies follow a relation between luminosity of the brightest young cluster and the star-formation rate…

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