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Extinction and Transformation: An Abstract

Published online by Cambridge University Press:  25 April 2016

Andrew T. Young
Andrew T. Young*
Affiliation:
Astronomy Department, San Diego State University San Diego, California 92182-0334

Extract

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The basic principles of heterochromatic extinction show that the approach used in the visible should not work well in the infrared, where molecular line absorption rather than continuous scattering dominates the extinction. Not only does this extinction change very rapidly with wavelength (so that stellar color becomes only weakly correlated with effective extinction), but also many of the lines are saturated (so that Forbe’s curve-of-growth effect is much more severe in the IR.) Furthermore, broadband IR colors are more undersampled than those in the visible, so aliasing errors make them correlate even less with extinction.

Type
Chapter V: Reports of Meetings of Commissions
Information
Transactions of the International Astronomical Union , Volume 20 , Issue 2 , 1988 , pp. 235 - 236
Copyright
Copyright © Kluwer 1988

References

Forbes, J.D. 1842, Phil. Trans. 132, 225–273 CrossRefGoogle Scholar
Manduca, A., and Bell, R.A. 1979, Pub. A.S.P. 91, 848 CrossRefGoogle Scholar
Manfroid, J., and Heck, A. 1983, Astron. Astrophys. 120, 302–306 CrossRefGoogle Scholar
Rufener, F. 1964, Pub. Obs. Geneve, Serie A, Fasc. 66 J7 Google Scholar
Young, A.T., and Irvine, W.M. 1967, Astron. J. 72, 945–950 CrossRefGoogle Scholar
Young, A.T. 1974, in Methods of Experimental Physics, Vol. 12 (Astrophysics, Part. A: Optical and Infrared), ed. by Carleton, N. (Academic Press, New York) pp. 123–192 CrossRefGoogle Scholar