Fig. 9.
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Line emissivities vs. depth for AGN and SF models, for three ζCR values of 10−14 s−1 (solid line), 10−13 s−1 (dash-dotted), and 10−12 s−1 (dotted), and two log U values of −3.0 (green) and −2.0 (blue). The teal-shaded area indicates the region where CRs heating becomes dominant. (a) [N II]λ6584 Å, AGN, nH = 100 cm−3. (b) [N II]λ6584 Å, AGN, nH = 103 cm−3. (c) [N II]λ6584 Å, SF, nH = 100 cm−3. (d) [S II]λλ6716,6731 Å, AGN, nH = 100 cm−3. (e) [S II]λλ6716,6731 Å, AGN, nH = 103 cm−3. (f) [S II]λλ6716,6731 Å, SF, nH = 100 cm−3. (g) [O I]λ6300 Å, AGN, nH = 100 cm−3. (h) [O I]λ6300 Å, AGN, nH = 103 cm−3. (i) [O I]λ6300 Å, SF, nH = 100 cm−3. (j) Hα, AGN, nH = 100 cm−3. (k) Hα, AGN, nH = 103 cm−3. (l) Hα, SF, nH = 100 cm−3.
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