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The IMF as a function of supersonic turbulence

C. Motta, P. Clark, S. Glover, R. Klessen, и A. Pasquali. (2016)cite arxiv:1608.01306Comment: 12 pages, 7 figures, accepted by MNRAS.
DOI: 10.1093/mnras/stw1921

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Massive blue early-type galaxies in the SDSS. I. A new population of recently quenched elliptical galaxiesD. McIntosh, C. Wagner, A. Cooper, E. Bell, D. Keres, F. Bosch, A. Gallazzi, T. Haines, J. Mann, A. Pasquali и 1 other автор(ы). (2013)cite arxiv:1308.0054Comment: 25 pages, 9 figures. Submitted to MNRAS. Version with full resolution figures at http://cas.umkc.edu/physics/mcintosh/mcintosh.RQE.hires.pdf.The Discovery of a Very Massive Star in W49S. Wu, A. Bik, T. Henning, A. Pasquali, W. Brandner, и A. Stolte. (2014)cite arxiv:1407.4804Comment: 5 pages, 3 figures, 1 table, accepted for publication in A&A Letters.The IMF as a function of supersonic turbulenceC. Motta, P. Clark, S. Glover, R. Klessen, и A. Pasquali. (2016)cite arxiv:1608.01306Comment: 12 pages, 7 figures, accepted by MNRAS.The Gas-Phase Metallicity of Central and Satellite Galaxies in the SDSSA. Pasquali, A. Gallazzi, и F. Bosch. (2012)cite arxiv:1206.3458Comment: 16 pages, 13 figures, accepted for publication in MNRAS.Bursty stellar populations and obscured active galactic nuclei in galaxy bulgesV. Wild, G. Kauffmann, T. Heckman, S. Charlot, G. Lemson, J. Brinchmann, T. Reichard, и A. Pasquali. Monthly Notices of the Royal Astronomical Society, 381 (2): 543--572 (2007)