Determination of Time Dependence in the Temperature Structure of Ionized Interstellar Gas

Details Determination of Time Dependence in the Temperature Structure of Ionized Interstellar Gas Determination of Time Dependence in the Temperature Structure of Ionized Interstellar Gas

Jun 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..390..111g&link_type=abstract

Pathways Through an Eclectic Universe ASP Conference Series, Vol. 390, proceedings of the conference held 23-27 April, 2007 at S

Astronomy and Astrophysics

Astronomy

Scientific paper

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 variable with time.

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