  I review the energy spectra of low mass X-ray binaries (LMXBs) containing
weakly magnetized accreting neutron stars (NS), emphasizing the most recent
broad band (0.1-200 keV) spectral and timing observations performed by
Beppo-SAX and RXTE. Drawing on the similarities between black hole candidate
(BHC) and NS accretion, I discuss the accretion geometry and emission processes
of NS LMXBs.
