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The Large Scale Structure of the X-Ray Universe

Published online by Cambridge University Press:  03 August 2017

X. Barcons  and
A.C. Fabian
X. Barcons
Affiliation:
Institute of Astronomy, Madingley Road, Cambridge CB3 OHA, United Kingdom
A.C. Fabian
Affiliation:
Institute of Astronomy, Madingley Road, Cambridge CB3 OHA, United Kingdom

Extract

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The clustering of the background-contributing X-ray sources is reflected in the excess (i.e., non-Poisson) fluctuations in the X-ray background (XRB). Observational limits on ΔI/I can therefore be used to constrain either the clumpiness of X-ray sources or their contribution to the XRB if their clustering properties are known (see Barcons & Fabian 1987 for details).

Type
Appendix 1: Poster Papers
Information
Symposium - International Astronomical Union , Volume 130: Large Scale Structures of the Universe , 1988 , pp. 539
Copyright
Copyright © Reidel 1988 

References

Barcons, X. & Fabian, A.C., 1987. Submitted to M.N.R.A.S. Google Scholar
Guilbert, P.W. & Fabian, A.C., 1986. M.N.R.A.S., 220, 439 Google Scholar
Shanks, T., Fong, R., Boyle, B.J. & Peterson, B.A., 1986. Preprint Google Scholar
Shafer, R.A. & Fabian, A.C., 1983. in IAU Symposium No. 104: Early Evolution of the Universe and its present structure. Ed. Abell, G.O. & Chincarini, G. Dordrecht:Reidel.Google Scholar