The magnetic field and the evolution of element spots on the surface of the HgMn eclipsing binary AR Aur
The system AR Aur is a young late B-type double-lined eclipsing binary with a primary star of HgMn peculiarity. We applied the Doppler imaging method to reconstruct the distribution of Fe and Y over the surface of the primary using spectroscopic time series obtained in 2005 and from 2008 October to...
| Autores: | , , , , , , , , , , , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2010 |
| País: | Argentina |
| Institución: | Consejo Nacional de Investigaciones Científicas y Técnicas |
| Repositorio: | CONICET Digital (CONICET) |
| Idioma: | inglés |
| OAI Identifier: | oai:ri.conicet.gov.ar:11336/12978 |
| Acceso en línea: | http://hdl.handle.net/11336/12978 |
| Access Level: | acceso abierto |
| Palabra clave: | STARS: ABUNDANCES BINARIES: ECLIPSING BINARIES: SPECTROCOPIC STARS: CHEMICALLY PECULIAR STARS: MAGNETIC FIELDS https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| Sumario: | The system AR Aur is a young late B-type double-lined eclipsing binary with a primary star of HgMn peculiarity. We applied the Doppler imaging method to reconstruct the distribution of Fe and Y over the surface of the primary using spectroscopic time series obtained in 2005 and from 2008 October to 2009 February. The results show a remarkable evolution of the element distribution and overabundances. Measurements of the magnetic field with the moment technique using several elements reveal the presence of a longitudinal magnetic field of the order of a few hundred gauss in both stellar components and a quadratic field of the order of 8 kG on the surface of the primary star. |
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