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Physical parameters of late M-type members of Chamaleon I and TW Hydrae Association: Dust settling, age dispersion and activity

, , , , , , , , and . (2016)cite arxiv:1610.06951Comment: 26 pages, 22 figures, 10 tables. Accepted in MNRAS.

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Planetesimal formation by sweep-up: how the bouncing barrier can be beneficial to growth, , , , , and . \aap, (April 2012)Messung des Hydratationsgrades der Haut mittels transkutaner nichtinvasiver Impedanzmessung, , , , and . Beiträge zur 38. Jahrestagung der Deutschen Gesellschaft für Biomedizinische Technik im VDE, DGBMT im VDE, (2004)The CARMENES search for exoplanets around M dwarfs: Nine new double-line spectroscopic binary stars, , , , , , , , , and 20 other author(s). (2018)cite arxiv:1808.06895Comment: Accepted for publication in A&A. 17 pages, 4 figures.Physical parameters of late M-type members of Chamaleon I and TW Hydrae Association: Dust settling, age dispersion and activity, , , , , , , , and . (2016)cite arxiv:1610.06951Comment: 26 pages, 22 figures, 10 tables. Accepted in MNRAS.Dynamical Habitability of Planetary Systems, , , , , , , , , and 15 other author(s). Astrobiology, (January 2010)A coagulation-fragmentation model for the turbulent growth and destruction of preplanetesimals, , , , and . \aap, (August 2008)The outcome of protoplanetary dust growth: pebbles, boulders, or planetesimals?. III. Sedimentation driven coagulation inside the snowline, , , and . \aap, (October 2011)Trapping solids at the inner edge of the dead zone: 3-D global MHD simulations, , , , and . \aap, (June 2010)Rapid planetesimal formation in turbulent circumstellar disks, , , , , and . \nat, (August 2007)The CARMENES search for exoplanets around M dwarfs: The warm super-Earths in twin orbits around the mid-type M dwarfs Ross 1020 (GJ 3779) and LP 819-052 (GJ 1265), , , , , , , , , and 20 other author(s). (2018)cite arxiv:1810.07572Comment: Accepted for publication in A&A. 15 pages, 12 figures, 4 tables.