Hostname: page-component-cd9895bd7-jkksz Total loading time: 0 Render date: 2024-12-26T03:48:16.116Z Has data issue: false hasContentIssue false

The Differential Polarization of Starlight as a Function of Distance

Published online by Cambridge University Press:  14 August 2015

Stephen Lloyd
Affiliation:
Center for Radiophysics and Space Research, Cornell University, Ithaca, N.Y. 14850, U.S.A.
Martin O. Harwit
Affiliation:
Center for Radiophysics and Space Research, Cornell University, Ithaca, N.Y. 14850, U.S.A.

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We have plotted the differential polarization as a function of distance and galactic longitude for 1732 stars between galactic latitudes −5° and +5°. The data were obtained from several published sources. A fairly clearcut distinction is seen between the effects of spiral arms and inter-arm regions indicating that starlight is systematically polarized only when passing through spiral arms.

Type
Part IV Interstellar Polarization
Copyright
Copyright © Reidel 1973 

References

Appenzeller, I.: 1966, Z. Atrophys. 64, 296.Google Scholar
Behr, A.: 1959, Veröff. U. Sternw. Göttingen , No. 126.Google Scholar
Bok, Bart J.: (1970) in De Jager, (ed.), Highlights of Astronomy , p. 63.Google Scholar
Hall, J. L.: 1958, Publ. U.S. Naval Obs. 2nd Ser. 17, No. VI.Google Scholar
Mathewson, D. S. and Ford, V. L.: 1970, Monthly Notices Roy. Astron. Soc. 74, 139.Google Scholar