Dusty discs as tracers of binary star formation.

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Scientific paper

The author reviews the recent observational and theoretical developments that make the study of circumbinary dust distributions particularly timely. First, he briefly describes the parameters of main sequence and of pre-main sequence binaries, paying particular attention to the properties of any associated gas/dust. Then, the author describes some recent theoretical work on binary-disc interactions and, finally, he discusses some of the issues that can be settled by future observational programmes.

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