Influence of Large-Scale Perturbations in Circumstellar Disks on the Linear Polarization Parameters of UX Ori Stars
- Авторы: Shulman S.G.1, Grinin V.P.1,2
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Учреждения:
- St. Petersburg State University
- Pulkovo Astronomical Observatory
- Выпуск: Том 45, № 10 (2019)
- Страницы: 664-676
- Раздел: Article
- URL: https://ogarev-online.ru/1063-7737/article/view/191586
- DOI: https://doi.org/10.1134/S1063773719100062
- ID: 191586
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Аннотация
The influence of large-scale perturbations in a circumstellar disk on the linear polarization of UX Ori stars is considered. We show that the position angle of the intrinsic linear polarization of a star surrounded by a geometrically thin flared disk cannot change significantly after the passage through the photometric minimum due to perturbations in the disk. In contrast, perturbations in a disk puffed up in the dust sublimation zone can give deflections of the plane of linear polarization of the system’s radiation up to 60°. This model allows the unusual changes in linear polarization observed in UX Ori and WW Vul after prolonged photometric minima to be explained.
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Об авторах
S. Shulman
St. Petersburg State University
Автор, ответственный за переписку.
Email: sgshulman@gmail.com
Россия, Universitetskii pr. 28, St. Petersburg, 198504
V. Grinin
St. Petersburg State University; Pulkovo Astronomical Observatory
Email: sgshulman@gmail.com
Россия, Universitetskii pr. 28, St. Petersburg, 198504; Pulkovskoe sh. 65, St. Petersburg, 196140
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