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Next: References Up: PAHs IN REFLECTION NEBULAE, Previous: IR signature in NGC7023

Conclusions

The numerous conclusions we were able to extract from the analysis of PAH and fullerene signatures in reflection nebulae are summarised here:

Acknowledgements: We are grateful to ESA member states for funding the ISO mission and instruments. Thanks to K. Uchida for providing the ISOCAM spectrum of VdB133. We gratefully acknowledge NATO Collaborative Research Grant 951347.
next up previous
Next: References Up: PAHs IN REFLECTION NEBULAE, Previous: IR signature in NGC7023

10/8/1998