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Disambiguation of "Burkert, Andreas"

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Declining rotation curves at $z=2$: A natural phenomenon in $Łambda$CDM cosmology

, , , , , , and . (2017)cite arxiv:1711.07985Comment: 6 pages, 4 figures, submitted to ApJ Letters, www.magneticum.org.

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Andreas Burkert

Andreas Burkert

Andreas Burkert

Andreas Burkert

Andreas Burkert

 

Other publications of authors with the same name

Fast Algorithm for Polygon Clipping with 3D Windows., and . Eurographics, North-Holland / Eurographics Association, (1988)Clipping an allgemeinen dreidimensionalen Polyedern.. Berichte aus der Informatik Shaker, (1994)The chemical evolution of local star forming galaxies: Radial profiles of ISM metallicity, gas mass, and stellar mass and constraints on galactic accretion and winds, , , , , , and . (2015)cite arxiv:1503.01503Comment: 19 pages, 17 figure, accepted to MNRAS.Instability of Supersonic Cold Streams Feeding Galaxies I: Linear Kelvin-Helmholtz Instability with Body Modes, , , , , , and . (2016)cite arxiv:1606.06289Comment: Final 10 pages are appendices. The main astrophysical figure is figure 11. Submitted to MNRAS.Bulge-forming galaxies with an extended rotating disk at z~2, , , , , , , , , and 17 other author(s). (2016)cite arxiv:1608.05412Comment: 10 pages, 5 figures, 2 tables, submitted to ApJ.The evolution of metallicity and metallicity gradients from z=2.7-0.6 with KMOS3D, , , , , , , , , and 21 other author(s). (2016)cite arxiv:1603.01139Comment: submitted to ApJ.Stellar feedback efficiencies: supernovae versus stellar winds, , , , , , , and . (Nov 16, 2015)Metallicity evolution at 0.8 < z < 2.6 from the LUCI, SINS/zC-SINF and KMOS-3D surveys, , , , , , , , , and 26 other author(s). (2014)cite arxiv:1405.6590Comment: 7 pages, 3 figures, submitted to ApJL.The Evolution and Origin of Ionized Gas Velocity Dispersion from $z\sim2.6$ to $z\sim0.6$ with KMOS$^3D$, , , , , , , , , and 20 other author(s). (2019)cite arxiv:1906.02737Comment: ~30 pages, 16 figures, 9 tables; accepted for publication in ApJ.Driving galactic winds with magnetic fields at low and high redshift, , , and . (2020)cite arxiv:2012.12905Comment: 21 pages, 9 Figures, comments very welcome, submitted to ApJ.