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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 2003 · astro-phShow all

6 papers · 2 filters

astro-ph2003

Evidence for a fundamental stellar upper mass limit from clustered star formation

Carsten Weidner, Pavel Kroupa

The observed masses of the most massive stars do not surpass about 150Msun. This may either be a fundamental upper mass limit which is defined by the physics of massive stars and/o…

astro-ph2003

On the origin of brown dwarfs and free-floating planetary mass objects

Pavel Kroupa, Jerome Bouvier

(abridged) Sub-stellar mass objects have fundamentally different binary properties than stars implying that they cannot have the same formation history. They are rather unfinished…

astro-ph2003

Massive Stars: Their Birth Sites and Distribution

Pavel Kroupa

The stellar IMF has been found to be an invariant Salpeter power-law (alpha=2.35) above about 1 Msun, but at the same time a massive star typically has more than one companion. Thi…

astro-ph2003

Galactic-Field IMFs of Massive Stars

Pavel Kroupa, Carsten Weidner

Over the past years observations of young and populous star clusters have shown that the stellar IMF appears to be an invariant featureless Salpeter power-law with an exponent alph…

astro-ph2003

On the universal outcome of star-formation: Is there a link between stars and brown-dwarfs?

P. Kroupa, J. Bouvier, G. Duchene +1

(abridged) The recent evidence obtained by Briceno et al. that star-formation in Taurus-Auriga (TA) may be producing significantly fewer brown dwarfs (BDs) per star than the ONC is…

astro-ph2003

The dynamical evolution of Taurus--Auriga-type aggregates

Pavel Kroupa, Jerome Bouvier

(abridged) Star formation in the Taurus--Auriga (TA) molecular clouds is producing binary-rich aggregates containing at most a few dozen systems within a region spanning one pc wit…