Modeling of large-scale disk perturbation eclipses of UX Ori stars with the puffed-up inner disks
Eclipses of UX Ori stars by compact gas–dust clouds and large-scale circumstellar disk perturbations are modeled. A flared disk and a disk with a puffing-up in the dust sublimation zone are considered. The disk puffing-up explains several observed features of eclipses. The linear polarization degree...
| Prif Awduron: | , |
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| Fformat: | Erthygl |
| Iaith: | English |
| Cyhoeddwyd: |
De Gruyter
2022-02-01
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| Cyfres: | Open Astronomy |
| Pynciau: | |
| Mynediad Ar-lein: | https://doi.org/10.1515/astro-2022-0010 |