SIMBAD references

The recently discovered coherent X-ray pulsations at a frequency of ∼400Hz in SAX J1808.4-3658, together with a measure of the source luminosity in quiescence, allow us to put an upper limit on the neutron star magnetic field, that is B≤5x10⁸ Gauss, using simple considerations on the position of the magnetospheric radius during quiescent periods. Combined with the lower limit inferred from the presence of X-ray pulsations, this constrains the SAX J1808.4-3658 neutron star magnetic field in the quite narrow range (1-5)x10⁸ Gauss. Similar considerations applied to the case of Aql X-1 give a neutron star magnetic field lower than ∼10⁹ Gauss.