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On the Determination of Physical Conditions in the Nebulae

Published online by Cambridge University Press:  14 August 2015

A.A. Boyarchuk ,
R.E. Gershberg ,
N.V. Godovnikov  and
V.I. Pronik
A.A. Boyarchuk
Affiliation:
Crimean Astrophysical Observatory, U.S.S.R.
R.E. Gershberg
Affiliation:
Crimean Astrophysical Observatory, U.S.S.R.
N.V. Godovnikov
Affiliation:
Crimean Astrophysical Observatory, U.S.S.R.
V.I. Pronik
Affiliation:
Crimean Astrophysical Observatory, U.S.S.R.

Extract

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Following the well-known physical theory of recombination and forbidden-line emission, we have carried out calculations which may be useful for a quantitative analysis of the observations of planetary nebulae and other emission objects (diffuse nebulae, emission details in extragalactic nebulae, symbiotic and flare stars). As the result, we have a set of four types of graphs.

Type
Session III – Physical Processes
Information
Symposium - International Astronomical Union , Volume 34: Planetary Nebulae , 1968 , pp. 162 - 165
Copyright
Copyright © Reidel 1968