  We examine the detectability through indirect means of weakly interacting
dark matter candidates that may constitute not all but only a subdominant
component of galactic cold dark matter. We show that the possibility of
indirect detection of neutralinos from their annihilations in the Earth and Sun
is not severely hampered by decreasing neutralino relic density. Upward-going
muon fluxes in underground detectors from neutralino annihilations in the Sun
can remain above the threshold of detectability of 10 muons/km^2/yr for
neutralinos composing 1% or more of the halo dark matter. Similarly, signals
from neutralino annihilations in the Earth can also remain high for neutralino
densities of 1% of the halo and actually would only be observable close to this
low density for neutralinos lighter than 150 GeV. We also show that there are
many models which simultaneously have high direct and indirect detection rates
making some model discrimination possible if a signal is seen in any of the
current dark matter searches.
