All Tables

• Table 1: Pulse period detections of SAX J2103.5+4545 with IBIS/ISGRI. The second column shows 0000the number of ScWs used for the computation in each epoch.
• Table 2: Orbital solution for SAX J2103.5+4545.
• Table 3: Comparison of the specific angular momentum of the accreted material to the Keplerian specific angular momentum at the magnetospheric radius. An estimation of the flux for the onset of centrifugal inhibition of accretion is also shown.