Reconnection X-winds: spin-down of low-mass protostars

We investigate the interaction of a protostellar magnetosphere with a large -scale magnetic field threading the surrounding accretion disc. It is assum ed that a stellar dynamo generates a dipolar-type field with its magnetic m oment aligned with the disc magnetic field. This leads to a magnetic neutra l line at the disc mid-plane and gives rise to magnetic reconnection, conve rting closed protostellar magnetic flux into open field lines. These are si multaneously loaded with disc material, which is then ejected in a powerful wind. This process efficiently brakes down the protostar to 10-20 per cent of the break-up velocity during the embedded phase.