Model emission spectra from primeval galaxies

Details Model emission spectra from primeval galaxies Model emission spectra from primeval galaxies

Dec 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...234..427s&link_type=abstract

Astrophysical Journal, Part 1, vol. 234, Dec. 1, 1979, p. 427-434.

Astronomy and Astrophysics

Astrophysics

51

Emission Spectra, Galactic Evolution, Stellar Evolution, Supernova Remnants, Ultraviolet Radiation, Abundance, Astronomical Models, Background Radiation, Cosmology, Diffuse Radiation, Radiative Transfer, Red Shift

Scientific paper

The paper computes models of the UV luminosity produced by a distribution of supernova remnants resulting from a burst of star formation in primeval galaxies at large redshift. The evolution of low metal abundance remnants is described analytically, and their UV emission is found from a velocity grid of radiative shock models. The implications of these results for the detection of line emission from young galaxies and for the diffuse background radiation are discussed.

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