IRAS observations of PN are presented and discussed, as well as ground based observations. The presentation and discussion of the data will highlight the general properties of the infrared emission of PN, with particular emphasis on the spatial distribution of the IR emission, on the energy distribution over the range 1 to 100 micron, and on some of the relevant properties of dust and ionized gas emission features.
- Pub Date:
- Galaxy: Planetary Nebulae;
- Planetary Nebulae: Infrared Spectra;
- Planetary Nebulae: Space Research