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ABSTRACT RECENTLY Prof. Fowler (Month. Not. Roy. Astr. Soc, December, 1912) has observed a number of new lines by passing a condensed discharge through mixtures of hydrogen and helium. Some
of these lines coincide closely with lines of the series observed by Pickering in the spectrum of the star ς Puppis, and attributed to hydrogen in consequence of its simple numerical
relation to the ordinary Balmer series. Other lines coincide closely with the series predicted by Rydberg and denoted as the principal series of the hydrogen spectrum. The rest of the new
lines show a very simple relation to those of the latter series, but apparently have no place in Rydberg's theory. Access through your institution Buy or subscribe This is a preview of
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INFORMATION AUTHORS AND AFFILIATIONS * The University, Copenhagen, N. BOHR Authors * N. BOHR View author publications You can also search for this author inPubMed Google Scholar RIGHTS AND
PERMISSIONS Reprints and permissions ABOUT THIS ARTICLE CITE THIS ARTICLE BOHR, N. _The Spectra of Helium and Hydrogen_ . _Nature_ 92, 231–232 (1913). https://doi.org/10.1038/092231d0
Download citation * Issue Date: 23 October 1913 * DOI: https://doi.org/10.1038/092231d0 SHARE THIS ARTICLE Anyone you share the following link with will be able to read this content: Get
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