direkt zum Inhalt springen

direkt zum Hauptnavigationsmenü

TU Berlin


warning: Creating default object from empty value in /www/Astro/etc/6/modules/i18n/i18ntaxonomy/i18ntaxonomy.pages.inc on line 34.

On the sub-grid modelling of turbulent dust foramtion in substellar atmospheres

Ch. Helling, R. Klein, P. Woitke, U. Nowak, and E. Sedlmayr

Astronomische Nachrichten, 324, 2 (2003)

Physical parameters of Bok Globules.

M. Hegmann, Ch. Hengel, M. Röllig, and W.H. Kegel

Astronomische Nachrichten, 324, 130 (2003)

Optical Constants and Extinction Efficiency of Solid materials

A. Tamanai, D. R. Alexander, J. W. Ferguson, and E. Sedlmayr

ASP Conf. Series, 288, 365(2003)

NLTE modelling of lines in expanding shells of LPVs

U. Bolick, He. Richter, and E. Sedlmayr

ASP Conf. Series, 288, 348(2003)

Opacities for protoplanetary discs

D. Semenov, Th. Henning, M. Ilgner, Ch. Helling, and E. Sedlmayr

ASP Conf. Series, 288, 361(2003)

Circuit of Dust in Substellar Objects

Ch. Helling

AG-Tagung: "The Cosmic Circuit of Matter", (2002)

Gzipped ps version (2.2 MB)


Dust formation in brown dwarf atmospheres under conditions of driven turbulence

Ch. Helling, R. Klein, P. Woitke, E. Sedlmayr

IAU Symposium No. 210 "Modelling of Stellar Atmospheres" (2002)

Gzipped ps version (812 KB)


Inhomogeneous Dust Formation due to Turbulent Motion in Brown Dwarf Atmospheres

Ch. Helling, M. Oevermann, M. Lüttke, E. Sedlmayr, R. Klein

4th Seminar: Euler & Navier-Stokes Equations: Theory, Numerical Solutien, Applications, 2001; eds. Kozel, Prihoda, Feistauer; p. 45

Gzipped PostScript version (240 KB)

Dust formation in turbulent media

Ch. Helling, M. Lüttke, E. Sedlmayr, R. Klein

Eighth International Conference on Hyperbolic Problems: Theory, Numerics, Applications (Feb. 2000)

Gzipped PostScript version (1.9 MB)


Mass loss characteristics of dust forming long-period variable stars

J.M. Winters, T. Le Bertre

Post-AGB objects (proto-planetary nebulae) as a phase of stellar evolution, eds. R. Szczerba and S.K. Gorny, p.93-100, Kluwer (2001)"

Gzipped PostScript version (83 KB)


Zusatzinformationen / Extras