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Astrophysics and Space Science

, Volume 154, Issue 1, pp 21–88 | Cite as

Planetary nebulae in the Galaxy

  • P. R. Amnuel
  • O. H. Guseinov
  • Yu. S. Rustamov
Article

Abstract

It is shown that the planetary nebulae can be divided into three types according to the values of the mass of shell and a central star. The criteria are given using which one can determine the mass type of the nebula. The distance scale of each mass-type planetary nebulae is given. The distribution of planetary nebulae in the Galaxy, their formation rate, scale-height and other physical and kinematic characteristics are investigated. A catalogue of planetary nebulae emitting in the radio range is given.

Keywords

Formation Rate Distance Scale Mass Type Kinematic Characteristic Radio Range 
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.

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Copyright information

© Kluwer Academic Publishers 1989

Authors and Affiliations

  • P. R. Amnuel
    • 1
  • O. H. Guseinov
    • 1
  • Yu. S. Rustamov
    • 1
  1. 1.Institute of PhysicsAcademy of SciencesBakuUSSR

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