Astronomy and Astrophysics – Astronomy
Scientific paper
May 1974
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974mmsai..45..109b&link_type=abstract
(Ministero della Pubblica Istruzione, CNR, and Universita di Trieste, European Regional Meeting in Astronomy, 2nd, Trieste, Ital
Astronomy and Astrophysics
Astronomy
1
Galactic Structure, Gaseous Diffusion, Interstellar Matter, Species Diffusion, Stellar Gravitation, Astronomical Models, Galactic Clusters, Interstellar Gas, Stellar Evolution, Stellar Spectra
Scientific paper
A two-phase model and a three-layer model are presented for the diffusion of interstellar matter in the Galaxy, in the framework of galactic evolution, with particular emphasis on the effects of microturbulent motion. The velocities of diffusion of the interstellar matter and the effects of diffusion in the intercloud medium are considered. Graphs are given for changes in the iron to hydrogen abundance ratio.
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