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Article Contents

ABSTRACT

1.INTRODUCTION

2.MODELLING THE COMPACT H II REGIONS

2.1.The Models

3.RESULTS

3.1.Continuum Emission From the Dust and the Gas

3.2.Spatial / Structural Information

3.3.Line Emission from the Gas

4.DISCUSSION

4.1.Mid Infrared Colours (PHT-P)

4.2.Far Infrared Colours (PHT-C)

4.3.Colour-Colour Plots (CCP)

4.3.1.Stellar Type O4

4.3.2.Stellar Type O7

4.3.3.Stellar Type B0.5

4.4.Radio Continuum to FIR Ratio

4.5.Structural Information

4.6.Information From the Line Emission

5.SUMMARY

REFERENCES