Centrum Astronomii
Wydział Fizyki, Astronomii i Informatyki Stosowanej, Uniwersytet Mikołaja Kopernika

An Accretor-Propeller Model of CH Cygni

Mikolajewski M., Mikolajewska J.

The authors propose a preliminary model of the activity of CH Cyg based on the theory of an oblique rotator (Lipunov 1987) and assuming an accreting white dwarf with magnetic axis nearly parallel to the rotational axis as the energy source of the hot component.