  The X-ray light curve and broad band spectral properties of the millisecond
X-ray pulsar/burster SAX J1808.4-3658 are reported. In the course of RXTE
observations in April--May 1998 the 3--150 keV luminosity of the source
decreased by a factor of ~100 from the peak value of ~9E36 erg/s (for a 4 kpc
distance). However, the spectrum was remarkably stable and maintained a roughly
power law shape with a photon index of ~2 without a strong high energy cut-off
below 100 keV, similar to that sometimes observed in the low spectral state of
X-ray bursters. An approximation of the averaged spectrum with an exponentially
cut-off power law with a superimposed reflected component yields the 90% lower
limit on the e-folding energy ~270 keV. We speculate that Comptonization on the
bulk motion in the radiation dominated shock might be a possible mechanism of
spectral formation. The decaying part of the X-ray light curve was cut off
abruptly at luminosity ~few 1E35 erg/s. Such behavior might be due to
centrifugal inhibition of accretion (transition to the ``propeller'' regime) as
well as to disk instability. In either case an upper limit on the neutron star
magnetic field strength is B < few 1E7 Gauss.

Astrophysics