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Interstellar Polarization in the Small Magellanic Cloud
Published online by Cambridge University Press: 07 August 2017
Abstract
Data of our on-going program on the interstellar polarization in the Small Magellanic Cloud (SMC) seem to show a correlation between the UV extinction and the parameters of the Serkowski law which describe the polarization. Fits of popular interstellar dust models to the polarization data are not always satisfactory, being better for stars with small wavelength of maximum polarization, λmax.
- Type
- External Galaxies
- Information
- Symposium - International Astronomical Union , Volume 150: Astrochemistry of Cosmic Phenomena , 1992 , pp. 109 - 110
- Copyright
- Copyright © Kluwer 1992