The generation of X-ray sources in close binary systems is studied. It is proposed that one of the stars is a white dwarf and it is accreting material from its companion. The entire treatment applies to the sphericaly symmetric and the stationary case. The model of this type accounts qualitatively for the observed nature of SCO X-1.
No takes yet. Share an insight, caveat, or question.
Reiun H oshi (1973) studied this question.