Accretion onto the neutron star in Be/X-ray binaries

We study accretion onto the neutron star in Be/X-ray binaries, using a 3D SPH code and the data imported from a high resolution simulation by Okazaki et al.
(2002) for a coplanar system with a short period ($P_{\mathrm{o}\mathrm{r}\mathrm{b}}=24.3\mathrm{d}$) and moderate eccentricity $(\mathrm{e}=0.34)$. We find that a time-dependent accretion disk is formed around the neutron star in Be/X-ray binaries. The disk shrinks after the periastron passage of the Be star and restores its radius afterwards. Our simulations show that the truncated Be disk model for Be/X-ray binaries is consistent with the observed X-ray behavior.