Determination of Time Dependence in the Temperature Structure of Ionized Interstellar Gas
It is well known that the temperature structure of ionized interstellar gas departs considerably from homogeneity. This is detected in the form of ``temperature fluctuations'' characterized by a parameter represented as t2. In this paper we present the formalism to check whether these small deviations from the equilibrium temperature are also
Giammanco, C. et al.
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2008