Seismic tests of the structure of rapidly oscillating Ap stars: HR 1217
HR 1217 is probably the best studied multiperiodic rapidly oscillating Ap star, which makes this star a test case for the seismic analysis of these complex stars. In this paper, we combine the observational data available for HR 1217 and use these data to constrain theoretical models appropriate for...
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| Outros Autores: | , |
| Formato: | article |
| Idioma: | eng |
| Publicado em: |
2003
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| Assuntos: | |
| Texto completo: | https://hdl.handle.net/10216/100606 |
| País: | Portugal |
| Oai: | oai:repositorio-aberto.up.pt:10216/100606 |