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TU Berlin


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)

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)

Gzipped postscript version (322 KB)


The IR-colour -- mass-loss relation of carbon-rich, dust-driven superwinds and a synthetic ( J-K, M_Bol) diagram

K.-P. Schröder, A. Wachter, and J.M. Winters

Astronomy & Astrophysics, 398, 229-237 (2003)

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Dust in brown dwarfs: II. The coupled problem of dust formation and sedimentation

P. Woitke and Ch. Helling

Astronomy & Astrophysics, 399, 297-313

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An improved mass-loss description for dust-driven superwinds and tip-AGB evolution models

A. Wachter, K.-P. Schröder, J.M. Winters, T.U. Arndt, and E. Sedlmayr

Astronomy & Astrophysics, 384, 452-459 (2002)

Gzipped pdf version (171 kB, A&A-Version)


On the shock-induced variability of emission lines in M-type Mira variables: I. Observational data

He. Richter and P.R. Wood

Astronomy & Astrophysics, 369, 1027-1047 (2001)

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Dust in brown dwarfs: I. Dust formation under turbulent conditions on microscopic scales

Ch. Helling, M. Oevermann, M. J. H. Lüttke, R. Klein and E. Sedlmayr

Astronomy & Astrophysics, 376, 194-212 (2001)

Gzipped PostScript version (2.1 MB)


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