Conclusions
The change in the nature of line broadening of the Hg 2537-Å line depends both on the density of metallic atoms and on the density of mercury atoms. It follows from this that for the systems Hg+Cd, Hg+Zn, and Hg+Mg the absorbing centers are weakly bound complexes of the type Hg+metal.
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Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Fizika, No. 2, pp. 130–131, February, 1975.
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Zav'yalova, A.Y., Zav'yalov, G.I. & Prilezhaeva, N.A. Broadening of the Hg 2537-Å line as a function of the density of Hg atoms in the presence of several metals. Soviet Physics Journal 18, 258–259 (1975). https://doi.org/10.1007/BF01103941
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DOI: https://doi.org/10.1007/BF01103941