INVESTIGATION OF THE INTERACTION BETWEEN THE PULSAR WIND AND THE BE-STAR DISK

PSR B125963 is a unique binary system with a radio pulsar from which unpulsedXray and radio emission was observed. The pulsar is in a highly eccentric 3.4year orbit with a Be star. The collision of the pulsar wind with the wind of Bestar plays a crucial role in the generation of the observed emission. The goalof this proposal is to investigate the changes of the system emission as thepulsar approaches to the Be star disk, and with the help of the received data toreconstruct the physical processes governing the system. truncated!, Please see actual data for full text [truncated!, Please see actual data for full text]