But not only the spatial distributions of
titanium and iron resemble those
in Cas A. Also the total amounts of these elements, their expansion velocities, and the velocity of the neutron star are
in amazing agreement with those of Cas A. «This ability to reproduce basic properties of the observations impressively confirms that Cas A may be the remnant of a neutrino - driven
supernova with its violent gas motions around the nascent neutron star,» concludes H. - Thomas Janka.
Using elaborate computer simulations, a team of researchers from RIKEN
in Japan and the Max Planck Institute for Astrophysics (MPA) were able to explain the recently measured spatial distributions of radioactive
titanium and nickel
in Cassiopeia A, a roughly 340 year old gas remnant of a nearby
supernova.