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Correlations between optical/near-infrared and UV extinction parameters and the prediction of UV extinction from ground-based photometryAn analysis of the variability of absolute UV extinction, A lambda derived through the ratio total-to-selective extinction, R Av/E(B-V), for 31 lines of sight for which UV extinction parameters were derived, is presented. For these data, which sample a wide range of environments and which are characterized by R = 2.5 to 6.0, differences in the shapes of UV extinction curves are largely due to variations in optical/near-UV extinction through changes in R. From this, it is found that UV extinction curves can be reproduced with reasonable accuracy by simply knowing R. Detection of an A2175/E(B-V) = 10 + or - 1 mag implies that the total extinction at 2175 A can be estimated from E(B-V) alone.
Document ID
19890007202
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Cardelli, Jason A.
(Wisconsin Univ. Madison, WI, United States)
Clayton, Goeffrey C.
(Wisconsin Univ. Madison, WI, United States)
Mathis, John S.
(Wisconsin Univ. Madison, WI, United States)
Date Acquired
September 5, 2013
Publication Date
June 1, 1988
Publication Information
Publication: ESA, Proceedings of the Celebratory Symposium on a Decade of UV Astronomy with the IUE Satellite, Volume 2
Subject Category
Astronomy
Accession Number
89N16573
Funding Number(s)
CONTRACT_GRANT: NAS5-26777
CONTRACT_GRANT: NAS7-918
CONTRACT_GRANT: NAG1-86
Distribution Limits
Public
Copyright
Other
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