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

Reach, W. T.; Wall, W. F.; Odegard, N.

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