Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982afz....18..143v&link_type=abstract
(Astrofizika, vol. 18, Jan.-Mar. 1982, p. 143-150.) Astrophysics, vol. 18, no. 1, July 1982, p. 86-90. Translation.
Astronomy and Astrophysics
Astronomy
4
Abundance, Cosmochemistry, Cosmology, Deuterium, Galactic Evolution, Cosmic Gases, Milky Way Galaxy, Radio Astronomy, Supernovae
Scientific paper
The change in the deuterium abundance during galactic evolution is considered. It is shown that the deuterium abundance observed in the present-day interstellar medium must correspond to the cosmological abundance. This conclusion does not depend on an assumption concerning the rate of accretion of intergalactic gas by the Galaxy. The change i the amount of deuterium by hypothetical pre-galactic supermassive objects is small. The importance of deuterium observations in the radio line D (wavelength = 91.6 cm) in absorption is noted.
Shchekinov Iu. A.
Vainer Boris V.
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