Continuous Emission in the Spectra of Gaseous Nebulae.

[en] The visual continua in the spectra of three nebulae photographed with a narrow slit are not produced by the blending of atomic emission lines but must have a physical origin. Several strong He I emission lines just beyond the Balmer limit may tend to vitiate measurements of the intensity distribution in the Balmer continuum on plates taken with a wide slit.

Disciplines :

Space science, astronomy & astrophysics

Author, co-author :

Swings, Polydore ; McDonald Observatory

Struve, Otto

Language :

English

Title :

Continuous Emission in the Spectra of Gaseous Nebulae.

Publication date :

1942

Journal title :

Astrophysical Journal

ISSN :

0004-637X

eISSN :

1538-4357

Publisher :

University of Chicago Press, Chicago, United States - Illinois

Volume :

Pages :

310-311

Additional URL :

http://adsabs.harvard.edu/abs/1942ApJ....96..310S

Available on ORBi :

since 16 September 2010

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