The potential of space observations for pulsating pre-main sequence stars
The first asteroseismic studies of pre-main sequence (pre-MS) pulsators have been conducted based on data from the space telescopes MOST and CoRoT with typical time bases of less than 40 days. With these data, a relation between the pulsational properties of pre-MS δ Scuti stars and their relative e...
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| Formato: | Artículo |
| Lenguaje: | English |
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EDP Sciences
2017-01-01
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| Colección: | EPJ Web of Conferences |
| Acceso en línea: | https://doi.org/10.1051/epjconf/201716003002 |