The transition region structure of κ ceti
Observations of κ Ceti (HD 20630), G5 V, obtained with the IUE satellite have been analysed to determine the structure of its outer atmosphere. This analysis is used to derive a model of transition region and to examine the terms of energy balance equation.
| Autores: | , , |
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| Tipo de recurso: | artículo |
| Fecha de publicación: | 1981 |
| País: | España |
| Institución: | Universidad Complutense de Madrid (UCM) |
| Repositorio: | Docta Complutense |
| Idioma: | inglés |
| OAI Identifier: | oai:docta.ucm.es:20.500.14352/64994 |
| Acceso en línea: | https://hdl.handle.net/20.500.14352/64994 |
| Access Level: | acceso abierto |
| Palabra clave: | 52 EUV spectra Stellar chromospheres Transition region Astrofísica Astronomía (Física) |
| Sumario: | Observations of κ Ceti (HD 20630), G5 V, obtained with the IUE satellite have been analysed to determine the structure of its outer atmosphere. This analysis is used to derive a model of transition region and to examine the terms of energy balance equation. |
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