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Rosseland and Plank mean opacities for protoplanetary discs

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

Astronomy & Astrophysics, 410, 611-621 (2003)

Dust in Brown Dwarfs II. The coupled problem of dust formation and sedimentation

P. Woitke, and Ch. Helling

Astronomy & Astrophysics, 399, 297-313 (2003)

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On the shock-induced variablity of emission linesin M-type Mira variables II. Fe II and Fe[II] emission lines as a diagnostic tool

He. Richter, P. R. Wood, P. Woitke, U. Bolick, and E. Sedlmayr

Astronomy & Astrophysics, 400, 319 (2003)

NLTE Modeling of Fe II and Fe[II] lines in the shocked atmospheres of M-type Miras

He. Richter, P. R. Wood, P. Woitke, U. Bolick, and E. Sedlmayr

ASP Conf. Proceedings, 288, 344 (2003)

High precision Monte Carlo radiative transfer in dusty media

G. Niccolini, P. Woitke, and B. Lopez,

Astronomy & Astrophysics, 399, 703-716 (2003)

Radiative transfer in clumpy environments: absorption and scattering by dust

M. Hegmann, and W.H. Kegel

MNRAS, 342, 453-462 (2003)

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Effects of correlated turbulent velocity fields on the formation of maser lines

R. Böger, W.H. Kegel, and M. Hegmann

Astronomy & Astrophysics, 406, 23-30 (2003)

Dust formation, grain growth and evaporation under the influence of temperature fluctuations

V. Schirrmacher and U. Dirks

Astronomische Nachrichten, 324, Suppl. Issue 3, p. 128 (2003)

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Self-consistent modeling of the outflow from the O-rich Mira IRC-20197

K.S. Jeong, J.M. Winters, T. Le Bertre, and E. Sedlmayr

Astronomy & Astrophysics, 407, 191-206 (2003)

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