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1 Introduction:
Line emission diagnostics in H II regions
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2 Inhomogeneities: The classical filling factor or optically thick
clumps?
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3 Calculations using FF and clumpy models
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4 Differences in the radial distributions of ionizing
and recombination photons between the FF and clumpy models
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5 Predictions of line strengths and ratios: Diagnostic diagrams for
density bounding
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6 Gas masses in H II regions
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7 Conclusions
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References
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