We report the discovery with BeppoSAX of a new 170.84 +/- 0.04s X-ray
pulsar, 1SAXJ1324.4-6200, found serendipitously in the field of the X-
ray binary XB 1323-619 in 1997 August. The source and periodicity are
also detected in archival ASCA data taken in 1994. The X-ray spectrum
is modeled by a power-law with a photon index of 1.0 +/- 0.4 and absor
ption of (7.8+/-(2.7)(1.1)) x 10(22) atom cm(-2). The source is locate
d close to the galactic plane and within 3' of the direction of the da
rk cloud DC 306.8+0.6. The measured interstellar absorption and cloud
size imply a distance >3.4 kpc. This implies a 1-10 keV source luminos
ity of >1.1 x 10(34) erg s(-1) during the BeppoSAX observation. The so
urce is not detected in earlier Einstein IPC and EXOSAT CMA observatio
ns, most probably due to reduced detector efficency and lower sensitiv
ity to highly absorbed sources. The X-ray properties suggest that 1SAX
J1324.4-6200 is an accreting neutron star with a Be star companion.