By combining a Serkowski-law interstellar polarization with four stellar polarization models, the authors show that UV spectropolarimetry can recover intrinsic stellar polarization where the interstellar signal is weakest.
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Analyzing Stellar and Interstellar Contributions to Polarization: Modeling Approaches for Hot Stars
By combining a Serkowski-law interstellar polarization with four stellar polarization models, the authors show that UV spectropolarimetry can recover intrinsic stellar polarization where the interstellar signal is weakest.