HD 161701, a chemically peculiar binary with a HgMn primary and an Ap secondary
In recent years, HgMn stars have attracted attention after in several of them surface chemical spots of different elements were discovered, whose origin and possible connection with binarity and magnetic fields is not clear yet. Aims. We perform a complete study of the HgMn binary HD 161701, includi...
| Autores: | , , , , , , , , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2013 |
| País: | Argentina |
| Institución: | Consejo Nacional de Investigaciones Científicas y Técnicas |
| Repositorio: | CONICET Digital (CONICET) |
| Idioma: | inglés |
| OAI Identifier: | oai:ri.conicet.gov.ar:11336/1640 |
| Acceso en línea: | http://hdl.handle.net/11336/1640 |
| Access Level: | acceso abierto |
| Palabra clave: | BINARYC CHEMICALLY PECULIAR STARS STARS ATMOSPHERES STARS ABUNDANCES MAGNETIC FIELD INDIVIDUAL (HD161701) SPECTROSCOPI https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| Sumario: | In recent years, HgMn stars have attracted attention after in several of them surface chemical spots of different elements were discovered, whose origin and possible connection with binarity and magnetic fields is not clear yet. Aims. We perform a complete study of the HgMn binary HD 161701, including the determination of physical parameters and photospheric chemical abundances. |
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