Far-ultraviolet extinction determined from Voyager data

Details Far-ultraviolet extinction determined from Voyager data Far-ultraviolet extinction determined from Voyager data

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...359l..23s&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 359, Aug. 10, 1990, p. L23-L27.

Astronomy and Astrophysics

Astrophysics

39

Cosmic Dust, Far Ultraviolet Radiation, Interstellar Extinction, Interstellar Matter, Ultraviolet Spectrometers, Voyager Project, Absorption Spectra, H I Regions, H Ii Regions, Line Spectra

Scientific paper

Data from the Voyager UV spectrometers are used to derive FUV extinction curves for 19 stars, using the pair-comparison method after the removal of the effects of line absorption due to H I and H2. It is shown that the FUV extinction rise continues to the limit of the data at about 925 A, supporting the theoretical prediction by Longo et al. (1989) that the FUV extinction continues to rise toward short wavelengths all the way to the Lyman limit at 912 A.

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