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Disambiguation of "Kroupa, Pavel"

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A discontinuity in the luminosity-mass relation and fluctuations in the evolutionary tracks of low-mass and low-metallicity stars at the Gaia M-dwarf gap

, and . (2021)cite arxiv:2104.13951Comment: Accepted to A&A.

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Pavel Kroupa

Ludwiga Kroupa

Dietrich Pavel

Wieland Werther Pavel

Jonas Philipp Pavelka

 

Other publications of authors with the same name

A perfect starburst cluster made in one go: the NGC 3603 young cluster, and . (2014)cite arxiv:1403.4601Comment: 9 pages, 6 figures. In press with The Astrophysical Journal.Has JWST already falsified dark-matter-driven galaxy formation?, , , and . (2022)cite arxiv:2210.14915Comment: Accepted for publication in ApJL, 10 pages, 4 figures, 1 tables.A new type of compact stellar population: dark star clusters, and . (2011)cite arxiv:1110.4103 Comment: 14 pages, 4 figures. Published in The Astrophysical Journal Letters.Runaway massive stars from R136: VFTS 682 is very likely a "slow runaway", , and . (2011)cite arxiv:1111.0291Comment: 21 pages (AASTeX preprint format), 4 figures, 4 tables, 2 online tables. Accepted for publication in The Astrophysical Journal.A discontinuity in the luminosity-mass relation and fluctuations in the evolutionary tracks of low-mass and low-metallicity stars at the Gaia M-dwarf gap, and . (2021)cite arxiv:2104.13951Comment: Accepted to A&A.Low-mass X-ray binaries indicate a top-heavy stellar initial mass function in ultra compact dwarf galaxies, , , and . (2011)cite arxiv:1110.2779 Comment: 18 pages, 8 figures, submitted to ApJ on August 15.The mmax-Mecl relation, the IMF and IGIMF: probabilistically sampled functions?, , and . (2013)cite arxiv:1306.1229Comment: 24 pages, 3 figures, 5 tables; accepted for publication by MNRAS.On the initial binary population for star cluster simulations, , , , and . (2017)cite arxiv:1707.04271Comment: 18 pages, 10 figures, 4 tables; accepted for publication in MNRAS.On the persistence of two small-scale problems in ŁambdaCDM, , , and . (Oct 27, 2015)Gas surface density, star formation rate surface density, and the maximum mass of young star clusters in a disk galaxy. II. The grand-design galaxy M51, , and . (2013)cite arxiv:1305.0558Comment: Abstract has been shortened; accepted for publication in ApJ.