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On the ultraviolet background radiation of the Galaxy

Published online by Cambridge University Press:  04 August 2017

A. Zvereva ,
A. Severny ,
L. Granitsky ,
G. Courtès ,
P. Cruvellier  and
C. T. Hua
A. Zvereva
Affiliation:
Crimean Astrophysical Observatory, Acad. Sci. USSR
A. Severny
Affiliation:
Crimean Astrophysical Observatory, Acad. Sci. USSR
L. Granitsky
Affiliation:
Crimean Astrophysical Observatory, Acad. Sci. USSR
G. Courtès
Affiliation:
Laboratoire d'Astronomie Spatiale du C.N.R.S. France
P. Cruvellier
Affiliation:
Laboratoire d'Astronomie Spatiale du C.N.R.S. France
C. T. Hua
Affiliation:
Laboratoire d'Astronomie Spatiale du C.N.R.S. France

Extract

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Observations of the far-UV spectrum (1300–1800 å) of the sky background at different galactic latitudes are presented. The measurements were made in deep space, at distances up to 2 × 105 km from the Earth with the photoelectric spectrometer (“Galaktika”) on board the “Prognoz-6” satellite. The highly elongated orbit of the satellite permitted corrections for scattered Lα-light. The contribution of stars was eliminated using fluxes measured in the TD-I and OAO-2 experiments.

Type
PART II: COMPOSITION, STRUCTURE AND KINEMATICS
Information
Symposium - International Astronomical Union , Volume 106: The Milky Way Galaxy , 1985 , pp. 237 - 238
Copyright
Copyright © Reidel 1985 

References

Severny, A.B., and Zvereva, A.M.: 1983, Astrophys. J. (Letters) 23, 71 Google Scholar
Shklovsky, I.S., and Sheffer, E.K.: 1971, Nature 231, 173 Google Scholar
Zvereva, A.M., Severny, A.B., Granitsky, L.V., Hua, C.T., Cruvellier, P., and Courtès, G.: 1982, Astron. Astrophys. 116, 312 Google Scholar