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The Far-Infrared Radiation in M83

Published online by Cambridge University Press:  12 April 2016

L. V. Jones  and
W. C. Keel
L. V. Jones
Affiliation:
University of Alabama, Dept. of Physics and Astronomy, Box 870324, Tuscaloosa, AL 34587
W. C. Keel
Affiliation:
University of Alabama, Dept. of Physics and Astronomy, Box 870324, Tuscaloosa, AL 34587

Extract

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The fact that a galaxy is barred may have an effect on the source of the far-infrared (FIR) radiation observed. Yet, to date, no one has addressed the effects that that might have on interpreting the global FIR signal. We hope to add to the existing data on FIR radiation in galactic bulges by comparing a barred galaxy, M83, to an unbarred galaxy, M74.

We use optical, Ha and UV images that are blurred to the same resolution as the IRAS HIRES images. Looking at the blurred UV images, bright "globs" were chosen and apertures were fit to them. The “globs” were then located on the optical, Hα and FIR images and fluxes were determined for each aperture used.

Type
Posters for Part I and Part II
Information
International Astronomical Union Colloquium , Volume 157: Barred Galaxies , 1996 , pp. 102 - 104
Copyright
Copyright © Astronomical Society of the Pacific 1996

References

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