Shock-Induced Polarized Hydrogen Emission Lines in the Mira Star omicron Ceti
In the spectra of pulsating stars, especially Mira stars, the detection of intense hydrogen emission lines has been explained by a radiative shock wave, periodically propagating throughout the atmosphere. Previous observation of the Mira star omicron Ceti around a bright maximum of light led to the...
| Main Authors: | , , |
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| Format: | Text |
| Language: | unknown |
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arXiv
2011
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| Subjects: | |
| Online Access: | https://dx.doi.org/10.48550/arxiv.1109.6500 https://arxiv.org/abs/1109.6500 |