Abstract
We present J, H, K, L photometry of a large sample (117) of objects classifed as planetary nebulae in the Perek - Kohoutec catalogue. According to the position of the sources in the near-IR colour-colour diagrams, we classify them in three classes: N (30%), D (13%), and S (57%). The energy distribution from 1 to 100μm is used to clarify the nature of S-type sources.
Based on observations collected at the European Southern Observatory (La Silla, Chile) and at the Italian Infrared Telescope (TIRGO).
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© 1987 D. Reidel Publishing Company
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Persi, P., Preite Martinez, A., Ferrari-Toniolo, M., Spinoglio, L. (1987). Near-Infrared Photometry of Iras Planetary Nebulae. In: Planetary and Proto-Planetary Nebulae: From IRAS to ISO. Astrophysics and Space Science Library, vol 135. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-3891-5_25
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DOI: https://doi.org/10.1007/978-94-009-3891-5_25
Publisher Name: Springer, Dordrecht
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