On the spectrum of neutral helium. Part II

dc.contributor.author	Raman, C.V.
dc.contributor.author	Ganesan, A.S.
dc.date.accessioned	2007-02-15T08:16:16Z
dc.date.available	2007-02-15T08:16:16Z
dc.date.issued	1924
dc.description	Open Access.	en
dc.description.abstract	A rejoinder to Dr. Silberstein's reply.- The two points raised by Dr. Silberstein in reply to the criticisms of his combination formula are answered. The figures have been recalculated, taking the maximum limit of the quantum numbers to the that proposed by Dr. Silberstein himself, and the number of fortuitous coincidences to be expected between the observed lines of the helium spectrum and those given by the formula is calculated and found to agree fairly well with the actual number. The view that the coincidences noticed are due to mere chance is maintained.	en
dc.format.extent	221193 bytes
dc.format.mimetype	application/pdf
dc.identifier.citation	Astrophysical Journal, 1924, Vol.59, p61-63	en
dc.identifier.issn	0004-637X
dc.identifier.issn	1538-4357 (online)
dc.identifier.uri	http://hdl.handle.net/2289/2156
dc.language.iso	en	en
dc.publisher	The University of Chicago Press for the American Astronomical Society	en
dc.relation.uri	http://adsabs.harvard.edu/cgi-bin/bib_query?1924ApJ....59...61R	en
dc.relation.uri	http://dx.doi.org/10.1086/142792	en
dc.rights	1989 American Astronomical Society. Scanned images provided by the NASA ADS Data System.	en
dc.title	On the spectrum of neutral helium. Part II	en
dc.type	Article	en

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