  We present a BeppoSAX observation of the X-ray source AX J0851.9-4617.4 that
has been proposed as the neutron star associated to the shell like-supernova
remnant RX J0852.0-4622. The image at E>5 keV shows the presence of a new
source, SAX J0852.0-4615, not resolved from AX J0851.9-4617.4 in previous
observations. The improved positional accuracy obtained for AX J0851.9-4617.4
confirms its possible identification with an early type star, also consistent
with its soft thermal spectrum (kT~1.3 keV). SAX J0852.0-4615, with a harder
X-ray spectrum and a higher X-ray to optical flux ratio, is a more likely
candidate for the neutron star associated to the supernova remnant.
