Protostars and Planets VI, Heidelberg, July 15-20, 2013

Poster 1S062

Molecular clouds, star formation, and a black hole

Lucas, William (University of St Andrews)
Bonnell, Ian (University of St Andrews)
Davies, Melvyn (Lund University)
Rice, Ken (University of Edinburgh)

Observations of the Galaxy’s centre have revealed the existence of two discs or possibly streamers of O and W-R stars orbiting Sgr A* at radii between about 0.05 and 0.5 pc and at an angle approaching 90° to one another. They are all roughly 6 million years old. This would indicate that two star forming gas discs arose from a single event. We use smoothed particle hydrodynamics (SPH) to show it is possible to create these from the infall of a single turbulent cloud, and then address how the infall itself may have come to pass.

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