activity
19962024
most citedA comprehensive set of simulations studying the influence of gas expulsion on star cluster evolution

417 citations · 5.4k across the 132 of their papers we have counts for

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Showing 2004 · astro-phShow all

7 papers · 2 filters

astro-ph2004★ 11 cited

The Fundamental Building Blocks of Galaxies

Pavel Kroupa

Most stars form in compact, dense embedded clusters with memberships ranging from a dozen stars to many millions of stars. Embedded clusters containing more than a few hundred star…

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

How star clusters could survive low star formation efficiencies

M. Fellhauer, P. Kroupa

After the stars of a new, embedded star cluster have formed they blow the remaining gas out of the cluster. Especially winds of high mass stars and definitely the on-set of the fir…

astro-ph2004

A Formation Scenario for the Heavy-Weight Cluster W3 in NGC 7252

M. Fellhauer, P. Kroupa

The young star cluster W3 (age 300-500 Myr) in NGC 7252 is the most luminous star cluster known to date. Dynamical mass estimates result in 8 +/- 2 * 10^7 M_sun. With an effective…

astro-ph2004

The Pleiades mass function: models versus observations

E. Moraux, P. Kroupa, J. Bouvier

Two stellar-dynamical models of binary-rich embedded proto-Orion-Nebula-type clusters that evolve to Pleiades-like clusters are studied with an emphasis on comparing the stellar ma…

astro-ph2004

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…