  We revisit Wyman's "other" scalar field solution of the Einstein equations
and its Sultana generalization to positive cosmological constant, which has a
finite 3-space and corresponds to a special case of a stiff fluid solution
proposed by Buchdahl and Land and, later, by Iba\~nez and Sanz to model
relativistic stars. However, there is a hidden cosmological constant and the
peculiar geometry prevents the use of this spacetime to model relativistic
stars.
