Simulated spectropolarimetry of accretion disc winds

We investigate how scattering varies across ADW spectral signatures, and we vary physical parameters, wind velocity laws and clumping. Our results are qualitatively similar to observations of a Nova-like CV suggesting that spectropolarimetry of ADW can help constrain CV parameters.</p><p> </p><p> </p><p>We applied our techniques to Broad Absorption Line Quasi Stellar Object (BALQSO) wind models and we investigated polarization across UV resonance lines and optical wind signatures.

Polarization levels in our simulations qualitatively match observations. </p> <p> </p><p>Our work suggests that spectropolarimetry is a powerful tool to probe ADW, revealing more about the underlying accretion continuum and how the wind kinematics and geometry may provide additional independent evidence to the spectrum from accreting objects. Thereby, enhancing knowledge about their driving mechanisms, mass-loss rates and ionization structure: highly important goals for the astronomical community.</p><br><i>Thesis is embargoed until 31st December 2029</i>.<br>