A new determination of the galactic electron temperature gradient for extended and low density ionized gas.

Astronomy and Astrophysics – Astronomy

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Electron Temperatures: H Ii Regions, Electron Temperatures: Galaxy

Scientific paper

By using electron temperature values derived from H166α recombination line and 1.4 GHz continuum observations of 19 H II regions, together with those given by Pedlar (1980) from H166α observations of low-density H II regions (with similar antenna beam) and a value of electron temperature given by Pedlar et al. (1978), a new determination of a galactic electron temperature gradient with the galactocentric distance is obtained for the low-density ionized gas.

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