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Influence of rotational darkening on ultraviolet interstellar extinction
Astronomische Nachrichten, 1989AbstractThe influence of rotational darkening on ultraviolet stellar fluxes of fast rotating stars has been rediscussed. For this aim ANS filter‐photometric magnitudes of weakly reddened B stars (E(B ‐ V) 0.1 mag) were corrected for interstellar extinction.
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Interstellar Extinction in the Ultraviolet from Celescope Observations
1974Celescope observations of 550 stars made in four broad ultraviolet passbands (1500 to 2600A) were used to derive intrinsic ultraviolet colors for main sequence stars (Haramundanis and Payne-Gaposchkin, 1973). Color excesses, E(Ui-V) = (Ui-V) — (Ui-V)O are qualitatively in agreement with those obtained by the Wisconsin Experiment (Bless and Savage, 1972)
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Empirical extinction coefficients for the Swift-UVOT optical-through-ultraviolet passbands
Monthly Notices of the Royal Astronomical Society, 2023Haibo Yuan, Ruoyi Zhang, Yuan Haibo
exaly
Extinction properties of ultrapure water down to deep ultraviolet wavelengths
Optical Materials Express, 2014Markus Schmidt
exaly
A survey of vacuum-ultraviolet extinction curves based on International Ultraviolet Explorer spectra
Monthly Notices of the Royal Astronomical Society, 1997S Aiello, Aiello S
exaly
Ultraviolet extinction toward a quiescent molecular cloud in the Small Magellanic Cloud
Astronomy and Astrophysics, 2012J Maíz Apellániz
exaly
Nano dust and the far ultraviolet extinction
Proceedings of the International Astronomical Union, 2018openaire +1 more source
Star formation and dust extinction properties of local galaxies from the AKARI-GALEX all-sky surveys
Astronomy and Astrophysics, 2010Tsutomu Takeuchi +2 more
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