Astronomy and Astrophysics – Astrophysics
Scientific paper
Jul 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979ap%26ss..63..379g&link_type=abstract
Astrophysics and Space Science, vol. 63, no. 2, July 1979, p. 379-387.
Astronomy and Astrophysics
Astrophysics
1
Distribution Functions, Interstellar Matter, Mass Spectra, Mass Transfer, Neutral Atoms, Nonlinearity, Calcium, Data Processing, Electron Density (Concentration), Frequency Distribution, Hydrogen Atoms, Inhomogeneity, Oort Cloud, Photoionization, Potassium
Scientific paper
Calculations by Penston (1969) of the mass distribution of interstellar clouds are analyzed using Hobb's data on the relationship between N(Ca II) and N(H). The simulation of the Oort cloud model is tested by drawing a graph of log(v) against log(I), where v is the mean velocity of the clouds and I is the line intensity. From this model it was determined that the adoption of a constant density model is not inconsistent with the equipartition of kinetic energy between the clouds. An extention of the Tarafdar (1978) model of a slab of gas with a normal radiation incident is made by taking a spherical cloud of constant density and integrating it over all directions to the surface of the clouds, assuming an isotropic surrounding radiation field.
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