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Interstellar Reddening at High Galactic Latitudes

Published online by Cambridge University Press:  14 August 2015

A. G. Davis Philip*
Affiliation:
Dudley Observatory and State University of New York at Albany, N.Y., U.S.A.

Abstract

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Measures in the Strömgren four-color and Hβ systems provide an accurate way to determine color excesses of early-type stars. Fourteen areas at high galactic latitude have now been searched for faint A stars which are then measured photoelectrically to obtain the color excesses. Non-main sequence A stars, which are easily detected by means of the four-color photometry, are not included in the analysis. Within 40° of each pole, the reddening is essentially zero, Eb–y = 0.00 north of the galactic plane and Eb–y = 0.01 south of the plane.

Type
Part V Distribution of Dust and Gas
Copyright
Copyright © Reidel 1973 

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