Far-ultraviolet diffuse galactic light

Details Far-ultraviolet diffuse galactic light Far-ultraviolet diffuse galactic light

Mar 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981apj...244l..69h&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 244, Mar. 1, 1981, p. L69-L72.

Astronomy and Astrophysics

Astrophysics

19

Diffuse Radiation, Far Ultraviolet Radiation, Galactic Radiation, Interstellar Matter, Light Scattering, Milky Way Galaxy, Albedo, Background Radiation, Calibrating, Radiation Distribution

Scientific paper

Diffuse galactic light is detected at very low galactic latitudes, and useful upper limits are obtained at moderate and high galactic latitudes. Together, these data indicate that the albedo of the interstellar grains is high (a greater than 0.5) and that the grains very strongly (g greater than 0.7) forward-scatter far-ultraviolet radiation.

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