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Tinbergen, J. Interstellar polarization in the immediate solar neighbourhood.
D.V.C. developed the data reduction code, carried out the data reductions, ran the ATLAS9 models and investigated Spica's interstellar polarization.
Serkowski, K., Mathewson, D. S. & Ford, V. L. Wavelength dependence of interstellar polarization and ratio of total to selective extinction.
We estimated the orientation of the interstellar polarization (ISP) at the position of SN 2007uy and, most interestingly, at the site of SN 2008D which has been subject of an intensive debate due to its possible connection with Gamma-Ray Bursts (GRBs).
The existence of interstellar polarization requires that interstellar grains must be nonspherical.
More than 70 years after the discovery of interstellar polarization, we now have a quantitative, empirically tested, theory of grain alignment giving ride to the observed effect.
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A composite dust grain model which simultaneously explains the observed interstellar extinction, polarization, IR emission and the abundance constraints, is required.
Cotton, D. V. et al. The intrinsic and interstellar broad-band linear polarization of nearby FGK dwarfs.
Another way in which the effects of interstellar dust become apparent is through the polarization of background starlight.
Local interstellar magnetic fields are poorly understood, but data showing weak polarization for nearby stars indicate dust may be trapped in fields or currents in the heliosheath nose region.
In this talk I will show how the E and B modes in the dust polarization are related to fluctuations in the magnetized interstellar medium.
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