|Title (1st Abstract)||
Runaway Stars in Supernova Remnants
Astrophysical Institute and University Observatory Jena, Germany
2. The search for the binary companions of SN progenitors in SNRs
Half of all stars and in particular 70 % of the massive stars are part of a multiple system. A possible development for the system after the core collapse supernova (SN) of the more massive component is as follows: The binary is disrupted by the SN. The formed neutron star is ejected by the SN kick whereas the companion star either remains within the system and is gravitationally bounded to the neutron star, or is ejected with a spatial velocity comparable to its former orbital velocity (up to 500 km/s). Such stars with a large peculiar space velocity are called runaway stars.
Astrophysical Institute and University Observatory Jena