Hostname: page-component-cd9895bd7-jn8rn Total loading time: 0 Render date: 2024-12-25T16:48:21.002Z Has data issue: false hasContentIssue false
  • English
  • Français

Infrared Energy Distribution of Selected Planetary Nebulae

Published online by Cambridge University Press:  19 July 2016

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

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Using the IRAS and near-IR photometry obtained at the 1-m, 3.6-m ESO telescopes, and 1.5-m TIRGO telescope, we will discuss the 1 - 100 microns energy distribution of selected PNe.

Type
I. Observational Data on Nebulae
Information
Symposium - International Astronomical Union , Volume 131: Planetary Nebulae , 1989 , pp. 57
Copyright
Copyright © Kluwer 1989