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Near Infrared Photometry of Compact Planetary Nebulae

  • M. Peña
  • S. Torres-Peimbert
Conference paper
Part of the International Astronomical Union / Union Astronomique Internationale book series (IAUS, volume 131)

Abstract

The study of young planetary nebulae can provide information about the ejection process of the nebular material as well as on nebular evolution and the enrichment of the interstellar medium. The youngest PN are expected to be compact and very dense, they usually show signs of variability and IR excess due to the presence of warm dust which, in some cases, seems to be mixed with the ionized gas.

Keywords

Interstellar Medium Extensive Program Infrared Emission Planetary Nebula Emission Mechanism 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

Copyright information

© International Astronomical Union 1989

Authors and Affiliations

  • M. Peña
    • 1
  • S. Torres-Peimbert
    • 1
  1. 1.Instituto de AstronomíaUniversidad Nacional Autónoma de MéxicoMéxico

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