Maser discs around massive young stars.

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Scientific paper

Observational evidence for the existence of maser discs around massive young stars is presented, with particular emphasis on sources with bipolar molecular outflows. In several cases molecular line data, indicate a massive disc or toroid orthogonal to the outflow, with OH masers tracing the inner (disrupted) portions of the disc, on scales of 1000 A.U. In Orion-KL H2O and SiO masers have been found to trace disc structure on scales smaller than 100 A.U.

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