III. On a cause for the appearance of bright lines in the spectra of irresolvable star-clusters | Zendy

Edward J. Stone | Zendy

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III. On a cause for the appearance of bright lines in the spectra of irresolvable star-clusters

Author(s) -

Edward J. Stone

Publication year - 1878

Publication title -

proceedings of the royal society of london

Language(s) - English

Resource type - Journals

eISSN - 2053-9126

pISSN - 0370-1662

DOI - 10.1098/rspl.1877.0072

Subject(s) - brightness , spectral line , star (game theory) , astrophysics , subject (documents) , physics , nuclear magnetic resonance , astronomy , computer science , library science

In the ‘Proceedings’ of the Royal Society for 1877, April 26, there is a short paper by Mr. Huggins, in which some views of mine on this subject are called in question. Mr. Huggins’s objections are threefold:- 1. “There are not found in the spectra of different nebulae the differences of relative brightness of the bright lines and of the continuous spectrum which would be expected on Mr. Stone s hypothesis.

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