1. Introduction
2. Observations
3. Spatial comparison to models
3.1 DEM L323: O3-4
3.1.1 U-sensitive diagnostics
3.1.2 T_*-sensitive diagnostics
3.1.3 Comparison to Hummer & Mihalas atmospheres
3.2 DEM L243: O7
3.2.1 Photoionization models
3.2.2 The SNR
3.3 DEM L199: Early WR
3.3.1 WR model atmospheres
3.3.2 Photoionization models
3.4 DEM L301: O3 shell
4. Spatially integrated spectra: T_* sequence
5. Conclusion
|