Exact nonstatic spherically symmetric solutions of the Einstein equati
ons for a null fluid source with pressure P and density rho related by
P=k rho(a) are given. The a=1 metrics are asymptotically flat for 1/2
<k less than or equal to 1 and cosmological for 0<k<1/2. The k=1 metri
c is the known charged Vaidya solution. In general the metrics have mu
ltiple apparent horizons. In the long time limit, the asymptotically f
lat metrics are hairy black hole solutions that ''fall between'' the S
chwarzschild and Reissner-Nordstrom metrics.