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Polarization Variability of Wolf-Rayet Binaries: Constraints on WR Parameters
Published online by Cambridge University Press: 03 August 2017
Extract
We have recently used the PISCO and VATPOL Polarimeters at the MPI (Chile) and CASLEO (Argentina) 2.2 m telescopes to monitor over several weeks the brightest WR+O systems fainter than 9th magnitude in the Galaxy (V filter) and LMC/SMC (GaAs tube without filter). Each data point is accurate to ~ 0.02% in polarization P.
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- Session IV. Binaries
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- Copyright © Kluwer 1991