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Three Possible Planetary Nebulae from Near-IR Observations

Published online by Cambridge University Press:  07 August 2017

P. Persi ,
A. Marenzi ,
A. Preite-Martinez  and
M. Ferrari-Toniolo
P. Persi
Affiliation:
Istituto di Astrofisica Spaziale, CP 67, 00044 Frascati, Italy
A. Marenzi
Affiliation:
Istituto di Astrofisica Spaziale, CP 67, 00044 Frascati, Italy
A. Preite-Martinez
Affiliation:
Istituto di Astrofisica Spaziale, CP 67, 00044 Frascati, Italy
M. Ferrari-Toniolo
Affiliation:
Istituto di Astrofisica Spaziale, CP 67, 00044 Frascati, Italy

Extract

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A catalogue of 388 new possible planetary nebulae was selected by Preite-Martinez (1988) from the IRAS Point Source Catalogue. These unidentified sources have IRAS colours in the range F(12)/F(25) ≤ 0.35 and F(25)/F(60) ≥ 0.35, and are located in the proximity of the galactic equator (|b| ≤ 15°). In order to identify these IRAS sources we have undertaken a programme of near-IR observations using an InSb photometer and a near-IR camera. We report here on results relative to four of these sources.

Type
I. The Observational PN Database
Information
Symposium - International Astronomical Union , Volume 155: Planetary Nebulae , 1993 , pp. 37
Copyright
Copyright © Kluwer 1993 

References

Persi, P., Preite-Martinez, A., Ferrari-Toniolo, M., Spinoglio, L. 1987, Planetary and protoplanetary nebulae: from IRAS to ISO , ed. Preite-Martinez, A., Reidel Pub. Co., p.221 CrossRefGoogle Scholar
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