Please use this identifier to cite or link to this item:
https://hdl.handle.net/10216/119418| Author(s): | Paola Angélica Quitral Manosalva |
| Title: | On using stellar pulsations to constrain atmospheric models of strongly magnetic stars |
| Issue Date: | 2019-03-06 |
| Subject: | Física Physical sciences |
| Scientific areas: | Ciências exactas e naturais::Física Natural sciences::Physical sciences |
| DOI: | 10.34626/f099-bc64 |
| TID identifier: | 101462069 |
| URI: | https://hdl.handle.net/10216/119418 |
| Document Type: | Tese |
| Rights: | openAccess |
| Appears in Collections: | FCUP - Tese |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| 323563.pdf | On using stellar pulsations to constrain atmospheric models of strongly magnetic stars | 14.47 MB | Adobe PDF |  View/Open |
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