Hostname: page-component-8448b6f56d-mp689 Total loading time: 0 Render date: 2024-04-24T12:27:04.308Z Has data issue: false hasContentIssue false
  • English
  • Français

A Limit on Galactic Extinction Not Correlated with Far IR Emission

Published online by Cambridge University Press:  12 April 2016

Douglas P. Finkbeiner ,
David J. Schlegel  and
Marc Davis
Douglas P. Finkbeiner
Affiliation:
University of California at Berkeley, Departments of Physics and Astronomy, 601 Campbell Hall, Berkeley, CA 94720
David J. Schlegel
Affiliation:
University of Durham, Department of Physics, South Road, Durham DH1 3LE, United Kingdom
Marc Davis
Affiliation:
University of California at Berkeley, Departments of Physics and Astronomy, 601 Campbell Hall, Berkeley, CA 94720

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.

We have reprocessed the IRAS and DIRBE full-sky 100 μm maps, using Hi as a zero-point, to produce a map of Galactic extinction. This map is crosscorrelated with APM galaxy counts over the full APM region, including dusty regions of the sky not used to compute the APM correlation function in Maddox et al.(1990a). The angular correlation function, w(θ), of galaxy counts is computed with and without the extinction correction, and is used to suggest that our map accounts for ~ 90% of the dust-induced correlation in the APM region on scales from 2 – 10°. This is the first time that a limit has been placed on the correlation function of the extinction not represented in a given map.

Type
Part VI Distant Hot Gas, SXRB Fluctuations, Dust, Gamma-rays
Information
International Astronomical Union Colloquium , Volume 166: The Local Bubble and Beyond , 1997 , pp. 367 - 370
Copyright
Copyright © Springer-Verlag 1998

References

Burstein, D. & Heiles, C. 1978, ApJ, 225, 40 Google Scholar
Burstein, D. & Heiles, C. 1982, AJ, 87, 1165 Google Scholar
Maddox, S.J., et al.l990a, MNRAS, 242, 43pGoogle Scholar
Maddox, S.J., et al.l990b, MNRAS, 243, 692 Google Scholar
Maddox, S.J., Efstathiou, G., & Sutherland, W.J. 1990c, MNRAS, 246, 433 Google Scholar
Hartmann, D. & Burton, W.B. 1996, Atlas of Galactic Neutral Hydrogen, Cambridge University Press.Google Scholar
Faber, S.M., et al.1989, ApJS, 69, 763 CrossRefGoogle Scholar
Heiles, C. 1976, ApJ, 204, 379 CrossRefGoogle Scholar
Santiago, B.X. 1996, et al.ApJ, 461, 38 Google Scholar
Saslaw, W.C. & Hamilton, A.J.S. 1984, ApJ, 276, 13 Google Scholar
Schlegel, D.J., Finkbeiner, D.P. and Davis, Marc 1998 in prepGoogle Scholar
Wheelock, S.L. et al. 1994, IRAS Sky Survey Atlas: Explanatory Supplement, JPL Publication 94-11 (Pasadena: JPL)Google Scholar