Abstract: | We consider the possible evolution of the rotation period and magnetic field of the X-ray source RX J0720.4-3125, assuming
that this source is an isolated neutron star accreting from the interstellar medium. The magnetic field of the source is estimated
to be 106–109 G (the most probable value is about 2·108 G), and it is difficult to explain the observed rotational period 8.38 s without invoking the hypothesis of magnetic field
decay. For calculations we used the model of ohmic dissipation of the field in the core of the neutron star. Estimates for
the accretion rate (10−14–10−16 M⊙/yr), velocity of the source through the interstellar medium (10–50 km/s), and neutron star age (2·109–1010 yrs) are obtained.
Lomonosov State University, Moscow, Russia; loffe Physical and Engineering Institute, St. Petersburg, Russia. Translated from
Izvestiya Vysshikh Uchebnykh Zavedenii, Radiofizika, Vol. 41, No. 1, pp. 28–35, January, 1998. |