Integral field spectroscopy of the planetary nebula NGC 3242 and the puzzling nature of its low-ionization structures

Open Access

Fig. 6

Detection of [C I] λ8727 at k1 and k4 LISs. The zoomed in figures show also the contours for the [O I] λ6300 (white) and [N I] λλ5198,5200 (magenta) emission lines. The images are smoothed with σ = 1.5. The color bar represents the values of the pixels (in flux units ×10⁻²⁰ erg s⁻¹ cm⁻² spaxel⁻¹).

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