Numerical calculations of the saturation behaviour of inhomogeneous cosmic masers

Details Numerical calculations of the saturation behaviour of inhomogeneous cosmic masers Numerical calculations of the saturation behaviour of inhomogeneous cosmic masers

Nov 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977a%26a....61..567b&link_type=abstract

Astronomy and Astrophysics, vol. 61, no. 4, Nov. 1977, p. 567-574. Research sponsored by the Deutsche Forschungsgemeinschaft.

Computer Science

Numerical Analysis

7

Astronomical Models, Interstellar Masers, Radiative Transfer, Iteration, Numerical Analysis, Radiant Flux Density, Saturation

Scientific paper

The saturation behavior of several models for inhomogeneous, spherical cosmic masers is numerically investigated. Our calculations give the values of the intensity and the center-to-limb variation of the emergent radiation, especially the dependence of these quantities on the density of the masing molecules and the pump parameter. Only when the masing molecules are confined to a very thin shell, the emitted radiation shows a shell structure, too.

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