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BN3 - Double Neutron Stars and Neutron Star-White Dwarf Binaries

Speaker

Tauris, Thomas

Coauthors

Talk Title

Ultra-stripped Supernovae and Double Neutron Star Systems

Abstract

The evolution of close-orbit progenitor binaries of double neutron star (DNS) systems leads to supernova (SN) explosions of ultra-stripped stars. The amount of SN ejecta mass is very limited from such, more or less, naked metal cores with envelope masses of only 0.01-0.2 Msun. The combination of little SN ejecta mass and the associated possibility of small NS kicks is quite important for the characteristics of the resulting DNS systems left behind. In this talk, I discuss theoretical predictions for DNS systems and compare with observations.

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