Prediction of the diffuse far-infrared flux from the galactic plane

Details Prediction of the diffuse far-infrared flux from the galactic plane Prediction of the diffuse far-infrared flux from the galactic plane

Jun 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976cosp.meetq....f&link_type=abstract

COSPAR, Plenary Meeting, 19th, Philadelphia, Pa., June 8-19, 1976, Paper. 18 p.

Astronomy and Astrophysics

Astronomy

Diffuse Radiation, Far Infrared Radiation, Galactic Radiation, Infrared Astronomy, Radiant Flux Density, Radiation Distribution, Astronomical Models, Carbon Monoxide, Cosmic Dust, Galactic Structure, Interstellar Gas, Molecular Gases

Scientific paper

A basic model and simple numerical relations useful for future far-infrared studies of the Galaxy are presented. Making use of recent CO and other galactic surveys, the diffuse far-infrared flux distribution from the galactic plane is predicted as a function of galactic longitude for longitudes between 4 and 90 deg; the far-infrared emissivity is predicted as a function of galactocentric distance. Future measurements of the galactic far-infrared flux would yield valuable information on the physical properties and distribution of dust and molecular clouds in the Galaxy, particularly the inner region.

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