Primeval galaxies

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Nov 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979sciam.241..130m&link_type=abstract

Scientific American, vol. 241, Nov. 1979, p. 130-134, 136, 138 (3ff.).

Astronomy and Astrophysics

Astronomy

Big Bang Cosmology, Galactic Evolution, Galactic Structure, Star Distribution, Black Holes (Astronomy), Interstellar Gas, Mass Distribution, Quasars, Red Shift, Schmidt Telescopes, Star Clusters, Stellar Luminosity, Stellar Mass, Stellar Spectra, Universe

Scientific paper

The paper presents theories on the evolution of galaxies, emphasizing a possible relationship between present and primeval galactic formations. A major problem, however, is the lack of instrumentation available for measuring galactic distances and spectra. Attention is given to determining a correlation between mass, luminosity, and lifetime of regular and primeval galaxies. Graphs are presented that depict the intrinsic excited spectrum of a primeval galaxy as well as the spectrum of a quasar. An attempt is made to determine the origin of quasars with the hope of discovering correlations with primeval and present galaxies.

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