“…The estimated formation-pressure conditions of the Olympias deposit are similar to those recorded in the lower pressure part of the "granite"-related Keno Hill, Canada (P: 468 675 bar), the lower-temperature distal (Erwood et al 1979 and data in Megaw et al 1988), Providencia, Mexico (Sawkins 1964 and data in Megaw et al 1988), Groundhog, USA (Meinert 1987), Washington Camp, USA (Surles 1978in Kwak 1986), Hidalgo, Mexico (Simone 1951in Kwak 1986), Uchucchacua, Peru (Bussel et al 1990), carbonate-replacement skarn-fi'ee Pb-Zn (Aq) deposits (Taebaek, Korea (So et al 1993), Bluebell, Canada (Ohmoto and Rye 1970), epithermal polymetallic Ag-Pb-Zn (Au) deposit {Creede, USA (Woods et al 1982 in Hedenquist and Henley 1985), Finlandia, Peru (Kamilli andOhmoto 1977, Sunnyside, USA (Casadeval and, and polymetallic Ag-Ph-Zn(Au) systems associated with "granitic" imrusions (Keno Hill, Canada (Lynch et al 1990) Beaverdell, Canada (Godwin et al 1986) with the Olympias deposit parts of skarn systems as in Providencia, Mexico (P: 300 bar), Naica, Mexico (P: 300 bar), and Groundhog, N. Mexico (P: 155-175 bar); and also the limestone replacement Bluebell, Canada (P: 300-800 bar), and Taebaek, Korea (P: 210-420 bar), and the epithermal Sunnyside, USA (P: 110 220 bar). The CO2 content of the Olympias inclusions is high enough to form a distinct liquid CO2 phase.…”