SDB Stars and the Structure of the Milky Way
Hot subdwarf stars are objects which are very suitable for studies of the older parts of our Galaxy. They belong to the brighter objects in such populations, and due to their blue colour and unique atmospheric properties they are easily found and unambigu
| Autores: | , , |
|---|---|
| Formato: | capítulo de livro |
| Estado: | Versión publicada |
| Fecha de publicación: | 2003 |
| País: | Chile |
| Idioma: | inglés |
| OAI Identifier: | oai:repositorio.anid.cl:10533/242401 |
| Acesso em linha: | https://hdl.handle.net/10533/242401 |
| Access Level: | acceso abierto |
| Resumo: | Hot subdwarf stars are objects which are very suitable for studies of the older parts of our Galaxy. They belong to the brighter objects in such populations, and due to their blue colour and unique atmospheric properties they are easily found and unambigu |
|---|