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Infrared Excess and Molecular Clouds: A Comparison of New Surveys of Far-Infrared and H I 21-cm Emission at High Latitudes

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dc.contributor.author Reach, W. T. en_US
dc.contributor.author Wall, W. F. en_US
dc.contributor.author Odegard, N. en_US
dc.date.accessioned 2004-09-24T20:19:52Z
dc.date.available 2004-09-24T20:19:52Z
dc.date.issued 1998-02 en_US
dc.identifier.citation Astrophysical Journal en_US
dc.identifier.citation USA en_US
dc.identifier.clearanceno 98-0331 en_US
dc.identifier.uri http://hdl.handle.net/2014/19111
dc.description.abstract We have created a map of the large-scale infrared surface bightness in excess of that associated with the atomic interstellar medium, using region-by-region correlations between the far-infrared and 21-cm line surface brightness. Our study updates and extends a previous attempt with the Infrared Astronomical Satellite and Berkeley/Parkes H I surveys. en_US
dc.format.extent 2645399 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other cosmology Diffuse Radiation Infrared ISM molecules molecular clouds en_US
dc.title Infrared Excess and Molecular Clouds: A Comparison of New Surveys of Far-Infrared and H I 21-cm Emission at High Latitudes en_US


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