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   PR # 43035
   We propose ASCA observations of two exceptional cooling-flows. The
   first, Abell 1068 (z = 0.139) has been shown through extensive ROSAT
   PSPC, optical and IRAS studies, to be shrouded in dusty, cold, X-ray
   absorbing material. ASCA observations will permit a detailed
   investigation of the properties of the cooling flow, its host
   cluster, and the nature of the absorbing gas. Deep ROSAT HRI and ISO
   observations of Abell 1068 are also scheduled and will complement the
   ASCA analysis. The second sour
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