Influence of Large-Scale Perturbations in Circumstellar Disks on the Linear Polarization Parameters of UX Ori Stars

被引:6
|
作者
Shulman, S. G. [1 ]
Grinin, V. P. [1 ,2 ]
机构
[1] St Petersburg State Univ, Univ Skii Pr 28, St Petersburg 198504, Russia
[2] Russian Acad Sci, Pulkovo Astron Observ, Pulkovskoe Sh 65, St Petersburg 196140, Russia
来源
ASTRONOMY LETTERS-A JOURNAL OF ASTRONOMY AND SPACE ASTROPHYSICS | 2019年 / 45卷 / 10期
关键词
variable stars; T Tauri; Herbig Ae; Be; circumstellar environment; radiative transfer; polarization; CENTRIFUGALLY DRIVEN WINDS; HERBIG AE/BE STARS; MIDINFRARED VARIABILITY; POLARIMETRIC ACTIVITY; PROTOSTELLAR DISKS; STELLAR OBJECTS; DEEP MINIMA; LIGHT; DUST; SCATTERING;
D O I
10.1134/S1063773719100062
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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 degrees. This model allows the unusual changes in linear polarization observed in UX Ori and WW Vul after prolonged photometric minima to be explained.
引用
收藏
页码:664 / 676
页数:13
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