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Fig. 5

image

Left: map of Te derived from the magnitude of the Paschen continuum jump at 8250 Å ratioed by the dereddened H I Paschen 11 (8862.8 Å) emission line strength. Initial estimates of Te and Ne from the [S III] and [Cl III] ratio maps were applied; see text for details. Low Te values over the two bright stars in the field (central star and field star to south-west) are produced by the stellar continua mimicking a low Te. Centre: map of the average temperature, T0. Right: map of the temperature fluctuation parameter, t2. Both were determined from the map presented in the left column and the Te ([S III]) map shown in Fig. 4.

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