On the theory of the large-scale distribution of interstellar matter in spiral galaxies

Details On the theory of the large-scale distribution of interstellar matter in spiral galaxies On the theory of the large-scale distribution of interstellar matter in spiral galaxies

May 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974mmsai..45...25r&link_type=abstract

(Ministero della Pubblica Istruzione, CNR, and Universita di Trieste, European Regional Meeting in Astronomy, 2nd, Trieste, Ital

Astronomy and Astrophysics

Astronomy

Density Wave Model, Galactic Evolution, Galactic Structure, Interstellar Matter, Spiral Galaxies, Star Distribution, Hubble Diagram, Interstellar Gas, Stellar Gravitation, Stellar Luminosity, Stellar Radiation

Scientific paper

The large-scale distribution of interstellar matter in spiral galaxies is studied on the basis of density-wave theory. The nonlinear response of the interstellar gas and the formation of galactic shock waves with two stable phases are investigated. The density-wave model is applied to a sample of twenty four external galaxies; a categorization is made of spiral galaxies; and the implications of the luminosity-class and Hubble-type of spiral galaxies are considered.

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