3D modeling of 1612 MHz OH masers: Monte Carlo modeling of the maser shells and the amplified stellar image

Astronomy and Astrophysics – Astrophysics

Scientific paper

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2 pages, 1 figure; to be published in: Proceeding of WS on Mass-Losing Pulsating Stars and their Circumstellar Matter, Sendai,

Scientific paper

We present the first results of our 3D Monte Carlo maser radiative transfer
code, used to model the 1612 MHz OH maser shell and the amplification of
emission from the stellar radio-photosphere.

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