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Cited article:

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Analyzing stellar and interstellar contributions to polarization: modeling approaches for hot stars

Richard Ignace, Andrew G. Fullard, Georgia V. Panopoulou, D. John Hillier, Christiana Erba and Paul A. Scowen
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Optimised use of interferometry, spectroscopy, and stellar atmosphere models for determining the fundamental parameters of stars

N. Ebrahimkutty, M. R. Gent, D. Mourard, A. Domiciano de Souza, M. Bergemann, T. Morel, G. Morello, N. Nardetto and B. Plez
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The effect of stellar contamination on low-resolution transmission spectroscopy: needs identified by NASA’s Exoplanet Exploration Program Study Analysis Group 21

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Influence of Thomson Electron Scattering Redistribution on Spectral Line Polarization Formed in Spherically Symmetric Extended and Expanding Atmospheres

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Modeling the Variable Polarization of ϵ Aurigae In and Out of Eclipse

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The inner dust shell of Betelgeuse detected by polarimetric aperture-masking interferometry

X. Haubois, B. Norris, P. G. Tuthill, et al.
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Polarimetry of transiting planets: Differences between plane-parallel and spherical host star atmosphere models

N. M. Kostogryz, T. M. Yakobchuk, S. V. Berdyugina and I. Milic
Astronomy & Astrophysics 601 A6 (2017)
https://doi.org/10.1051/0004-6361/201628762