Hostname: page-component-cd9895bd7-fscjk Total loading time: 0 Render date: 2024-12-26T04:59:10.681Z Has data issue: false hasContentIssue false
  • English
  • Français

Observations of the Diffuse Ultraviolet Background from the UVX Experiment On Space Shuttle

Published online by Cambridge University Press:  08 February 2017

Richard C. Henry ,
Paul D. Feldman  and
Jayant Murthy
Richard C. Henry
Affiliation:
Department of Physics and Astronomy The Johns Hopkins University Baltimore, MD 21218, USA
Paul D. Feldman
Affiliation:
Department of Physics and Astronomy The Johns Hopkins University Baltimore, MD 21218, USA
Jayant Murthy
Affiliation:
Laboratory for Astronomy and Solar Physics Goddard Space Flight Center MD 20771, USA

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The UVX experiment has resulted in confirmation that the diffuse ultraviolet background is low in intensity everywhere and that it is fairly uniform in intensity, both spatially and spectrally. There is no clear evidence that any significant portion of the moderate galactic latitude diffuse cosmic background originates in galactic plane starlight scattering from interstellar dust.

Type
III. Diffuse Galactic Radiation from Dust and Gas: Observations and Models
Information
Symposium - International Astronomical Union , Volume 139: The Galactic and Extragalactic Background Radiation , 1990 , pp. 227 - 228
Copyright
Copyright © Kluwer 1990 

References

REFERENCES

Anderson, R. C., Henry, R. C., and Fastie, W. G. 1982, Ap. J., 259, 573.CrossRefGoogle Scholar
Joubert, M., Masnou, J. L., Lequeux, J., Deharveng, J. M., and Cruvellier, P. 1983, Astr. Ap., 128, 114.Google Scholar
Murthy, J., Henry, R. C., Feldman, P. D., and Tennyson, P. D. 1989a, Ap. J., 336, 954.CrossRefGoogle Scholar
Murthy, J., Henry, R. C., Feldman, P. D., and Tennyson, P. D. 1989b, Astr. Ap., (in press).Google Scholar
Paresce, F., Jakobsen, P., and Bowyer, S. 1983, Astr. Ap., 124, 300.Google Scholar
Paresce, F., Margon, B., Bowyer, S., and Lampton, M. 1979, Ap. J., 230, 304.CrossRefGoogle Scholar
Paresce, F., McKee, C., and Bowyer, S. 1980, Ap. J., 240, 387.CrossRefGoogle Scholar
Weller, C. S. 1983, Ap. J., 268, 899.CrossRefGoogle Scholar