The density profile and the wavelength dependence of compact radio source size

Astronomy and Astrophysics – Astrophysics

Scientific paper

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4 pages

Scientific paper

In the gaseous disk model, the density profile is derived from the mass and
energy conservation in the gravitational field of a central energy source.
Using the condition for emission, following from the induced character of
radiation process, we obtain the wavelength dependence of radio source size
which is consistent with observational data.

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