  We report a series of numerical simulations showing that the critical
magnetic Reynolds number Rm_c for the nonhelical small-scale dynamo depends on
the Reynolds number Re. Namely, the dynamo is shut down if the magnetic Prandtl
number Pr=Rm/Re is less than some critical value Pr_c<1 even for Rm for which
dynamo exists at Pr>=1. We argue that, in the limit of Re->infinity, a finite
Pr_c may exist. The second possibility is that Pr_c->0 as Re->infinity, while
Rm_c tends to a very large constant value inaccessible at current resolutions.
If there is a finite Pr_c, the dynamo is sustainable only if magnetic fields
can exist at scales smaller than the flow scale, i.e., it is always effectively
a large-Pr dynamo. If there is a finite Rm_c, our results provide a lower
bound: Rm_c<220 for Pr<=1/8. This is larger than Rm in many planets and in all
liquid-metal experiments.
