Interstellar extinction in the UV

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ID: 300655
1979
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Ranked #469 of 1,339 articles by views in monthly notices of the royal astronomical society

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Abstract
The UV interstellar extinction obtained from observations using the OAO-2, Copernicus and TD-1 satellites, is fitted to simple analytical expressions in the variable x = 1/λ. The feature centred at |$\lambda \simeq 2200$| Å can be fitted to a Lorentz profile; this result may be of physical significance.
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openalex_W2004645596 Use this key to autocite in the manuscript while using SciMatic Manuscript Manager or Thesis Manager
Authors
Journal monthly notices of the royal astronomical society
Year 1979
DOI
10.1093/mnras/187.1.73p
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