Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/2156
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dc.contributor.authorRaman, C.V.-
dc.contributor.authorGanesan, A.S.-
dc.date.accessioned2007-02-15T08:16:16Z-
dc.date.available2007-02-15T08:16:16Z-
dc.date.issued1924-
dc.identifier.citationAstrophysical Journal, 1924, Vol.59, p61-63en
dc.identifier.issn0004-637X-
dc.identifier.issn1538-4357 (online)-
dc.identifier.urihttp://hdl.handle.net/2289/2156-
dc.descriptionOpen Access.en
dc.description.abstractA 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.extent221193 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherThe University of Chicago Press for the American Astronomical Societyen
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/bib_query?1924ApJ....59...61Ren
dc.relation.urihttp://dx.doi.org/10.1086/142792en
dc.rights1989 American Astronomical Society. Scanned images provided by the NASA ADS Data System.en
dc.titleOn the spectrum of neutral helium. Part IIen
dc.typeArticleen
Appears in Collections:C.V. Raman - Scientific Papers, Vol.3. Optics

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