  While model-independent limits are always interesting, a limit on neutron
star radius as a function of mass attains special interest in light of recent
interpretations of the periodic as well as quasi-periodic oscillations (QPOs)
in brightness of X-rays emitted from neutron stars that are accreting matter
from a low-mass companion. Here we derive such a limit based only on well
accepted principles. We discuss our limit in connection with a recent
interpretation of X-ray pulsations from SAX J1808.4-3658 as indicating a
strange-star candidate, and show that this object can also be a normal neutron
star, though one whose central core has very high density. The most plausible
high-density phase of hadronic matter, which is also expected to be very
compressible, is quark matter. So an alternative to the strange star
interpretation of SAX J1808.4-3658 is that it is a hybrid neutron star.
