Continuous Spectrum of Nova Herculis

Details Continuous Spectrum of Nova Herculis Continuous Spectrum of Nova Herculis

Mar 1936

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1936natur.137..405g&link_type=abstract

Nature, Volume 137, Issue 3462, pp. 405-406 (1936).

Physics

1

Scientific paper

IN NATURE of January 25, p. 150, Dr. W. M. Cohn refers to the spectrophotometric observations of Nova Herculis 1934 by Barbier, Chalonge and Vasy. In the earlier stages of the Nova these investigators find a secondary maximum in the energy distribution of the continuous spectrum, and Dr. Cohn attributes this feature to electron radiation, and deduces that ``the early stage of a nova seems to permit the generation of free electrons of high speed''.

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