Assuming that a given speleothem precipitates near
thermodynamic equilibrium, quantitative interpretation of its
^(18)O record in terms of physical parameters is generally
hampered by the lack of robust methods for separating
isotopic variations due to paleo-temperatures and those
reflecting source water composition. Moreover, in many
settings it appears likely that speleothems form out of
equilibrium, due to kinetic isotopic fractionation caused by
rapid CO_2 degassing, which further detracts from the
reliability of paleo-environmental reconstructions