Interstellar extinction in the UV

Details Interstellar extinction in the UV Interstellar extinction in the UV

Jun 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979mnras.187p..73s&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 187, June 1979, p. 73P-76P.

Astronomy and Astrophysics

Astronomy

1336

Astronomical Spectroscopy, Interstellar Extinction, Satellite Observation, Ultraviolet Astronomy, Oao 2, Oao 3, Spectrophotometry, Td-1 Satellite, Ultraviolet Spectroscopy

Scientific paper

The UV interstellar extinction obtained from observations with the OAO
2, Copernicus, and TD 1 satellites is fitted to simple analytical
expressions in the variable x = 1/lambda. The feature centered at a
wavelength of about 2200 A can be fitted to a Lorentz profile; this
result may be of physical significance.

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