270. WE-Heraeus Seminar on Neutron Stars, Pulsars and Supernova Remnants

By W. Becker, H. Lesch, J. Trümper. 2002

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Physics of strongly magnetized neutron stars (2006, methodology): “Further works used improved opacity and equation of state data from the OPAL project for pure hydrogen, helium and iron compositions (Rajagopal and Romani 1996, Zavlin et al 1996, Gänsicke et al 2002, Pons et al 2002).”
Non-spherical core collapse supernovae. I. Neutrino-driven convection, Rayleigh-Taylor instabilities, and the formation and propagation of metal clumps (2003, methodology): “On the other hand Aschenbach (2002) and Aschenbach et al. (1995) deduce low mean expansion velocities of about 2000km s −1 for the clumps in the Vela supernova remnant (using their angular distance to the pulsar, the age of the latter and the distance of the remnant), that are in reasonably good agr”