We report RossiXTE and BeppoSAX observations of the X-ray pulsar RX J0146.9
+6121, the neutron star/Be binary system with the longest known spin period
.
Data obtained one month after the most recent outburst (July 1997), show th
at the source has returned to its normal luminosity of a few 10(34) erg s(-
1) while spin-up continued at an average rate of similar to 5 x 10(-8) s s(
-1).