The behaviour of fast rotating neutron stars in binary systems https://www.mpg.de/5011886/millisecond_pulsars
Numerical calculations on the base of stellar evolution and accretion torques, demonstrating how millisecond pulsars loose about half of their rotational energy during the final stages of the mass-transfer process before the pulsar turns on its radio beam.
Astronomy group at the Max Planck Institute for Radio Astronomy (led by Michael Kramer