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The Galactic Far-UV Background: Correlations with Gas and Dust at High Galactic Latitudes

Published online by Cambridge University Press:  08 February 2017

James Lequeux
James Lequeux*
Affiliation:
Radioastronomie, ENS 24 rue Lhomond 75231 Paris Cedex 05, France and Paris-Meudon Observatory

Abstract

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The correlations between the UV galactic background (after subtraction of direct starlight), the neutral hydrogen HI, the extinction and the 100 μm emission are discussed for high galactic latitudes mainly based on a new analysis of the D2B satellite data. While clear correlations exist between UV and the other quantities, indicating that most of the UV galactic background is starlight scattered by interstellar dust, these correlations are less tight than the correlation between HI and the 100 μm emission. Localized UV excesses are shown to exist and are due in some cases to 2-photon emission by ionized gas. The quantitative interpretation of the UV galactic background in terms of dust properties is discussed, and it is shown that both the galactic model and the clumpiness of interstellar radiation may affect the results considerably.

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. 185 - 192
Copyright
Copyright © Kluwer 1990 

References

REFERENCES

Boissé, P. 1989, Astron. Astrophys., in press.Google Scholar
Boulanger, F. 1989, in Proc. IAU 139, Galactic and Extragalactic Background Radiation, ed. Bowyer, S. and Leinert, Ch. (Dordrecht: Kluwer Academic Publishers).Google Scholar
Boulanger, F., and Pérault, M. 1988, Astrophys. J. 330, 964.CrossRefGoogle Scholar
Bowyer, S. 1989, in Proc. IAU 139, Galactic and Extragalactic Background Radiation, ed. Bowyer, S. and Leinert, Ch. (Dordrecht: Kluwer Academic Publishers).Google Scholar
Burstein, D., and Heiles, C. 1978, Astrophys. J. 225, 40.CrossRefGoogle Scholar
Caplan, J. and Grec, G. 1979, Astron. Astrophys., 78, 335.Google Scholar
Désert, F.X., Basell, D. and Boulanger, F. 1988, Astrophys. J., 334, 815.CrossRefGoogle Scholar
Fix, J. D., Graven, J. D., and Frank, L. A. 1989, in Proc. IAU 139, Galactic and Extragalactic Background Radiation, ed. Bowyer, S. and Leinert, Ch. (Dordrecht: Kluwer Academic Publishers).Google Scholar
Guhathakurta, P., and Tyson, A. 1989, in Proc. IAU 139, Galactic and Extragalactic Background Radiation, ed. Bowyer, S. and Leinert, Ch. (Dordrecht: Kluwer Academic Publishers).Google Scholar
Henry, R. C., Murthy, J., and Feldman, P. D. 1989, in Proc. IAU 139, Galactic and Extragalactic Background Radiation, ed. Bowyer, S. and Leinert, Ch. (Dordrecht: Kluwer Academic Publishers).Google Scholar
Hurwitz, M., Bowyer, S., and Martin, C. 1989, in Proc. IAU 139, Galactic and Extragalactic Background Radiation, ed. Bowyer, S. and Leinert, Ch. (Dordrecht: Kluwer Academic Publishers).Google Scholar
Jacobsen, P., de Vries, J.S., and Paresce, F. 1987, Astron. Astrophys. 183, 335.Google Scholar
Joubert, M., Masnou, J.L., Lequeux, J., Deharveng, J.M., and Cruvellier, P. 1983, Astron. Astrophys. 128, 114.Google Scholar
Kiszkurno-Koziej, E., and Lequeux, J. 1987, Astron. Astrophys. 185, 291.Google Scholar
Lebrun, F. 1986, Astrophys. J. 306, 16.CrossRefGoogle Scholar
Lockman, F.J., Jahoda, K., and McCammon, D. 1986, Astrophys. J. 302, 432.CrossRefGoogle Scholar
Magnani, L., Blitz, L., and Mundy, L. 1985, Astrophys. J. 295, 402.CrossRefGoogle Scholar
Martin, C., Hurwitz, M., and Bowyer, S. 1989, in Proc. IAU 139, Galactic and Extragalactic Radiation, ed. Bowyer, S. and Leinert, Ch. (Dordrecht: Kluwer Academic Publishers).Google Scholar
Mattila, K. 1971, Astron. Astrophys. 15, 292.Google Scholar
Maucherat-Joubert, M., Cruvellier, P., and Deharveng, J. M. 1979, Astron. Astrophys. 74, 218.Google Scholar
Maucherat-Joubert, M., Deharveng, J. M., and Cruvellier, P. 1980, Astron. Astrophys. 88, 323.Google Scholar
Mebold, U., Cernicharo, J., Velden, L., Reif, K., Crezelius, C., and Goerigk, W. 1985, Astron. Astrophys. 151, 427 Google Scholar
Paresce, F. 1989, in Proc. IAU 139, Galactic and Extragalactic Background Radiation, ed. Bowyer, S. and Leinert, Ch. (Dordrecht: Kluwer Academic Publishers).Google Scholar
Reach, W., Heiles, C., and Koo, B.C. 1989, in Proc. IAU 139, Galactic and Extragalactic Background Radiation, ed. Bowyer, S. and Leinert, Ch. (Dordrecht: Kluwer Academic Publishers).Google Scholar
Reynolds, R. J. 1985, Astron. J. 90, 92.CrossRefGoogle Scholar
Stark, A. A., Bally, J., Linke, R. A., and Heiles, C. 1989, unpublished. The magnetic tape containing the survey can be obtained from Dr. Stark.Google Scholar
Strong, A. W., and Lebrun, F. 1982, Astron. Astrophys. 105, 159.Google Scholar
Witt, A. N. 1989 in, Proc. IAU 139, Galactic and Extragalactic Background Radiation, ed. Bowyer, S. and Leinert, Ch. (Dordrecht: Kluwer Academic Publishers).Google Scholar