Searching for a link between the presence of chemical spots on the surface of HgMn stars and their weak magnetic fields
We present the results of mapping the HgMn star AR Aur using the Doppler Imaging technique for several elements and discuss the obtained distributions in the framework of a magnetic field topology.
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| Veröffentlicht in: | Proceedings of the International Astronomical Union 2008-11, Vol.4 (S259), p.401-402 |
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| container_end_page | 402 |
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| container_issue | S259 |
| container_start_page | 401 |
| container_title | Proceedings of the International Astronomical Union |
| container_volume | 4 |
| creator | Savanov, Igor S. Hubrig, S. González, J. F. Schöller, M. |
| description | We present the results of mapping the HgMn star AR Aur using the Doppler Imaging technique for several elements and discuss the obtained distributions in the framework of a magnetic field topology. |
| doi_str_mv | 10.1017/S1743921309030865 |
| format | Article |
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| ispartof | Proceedings of the International Astronomical Union, 2008-11, Vol.4 (S259), p.401-402 |
| issn | 1743-9213 1743-9221 |
| language | eng |
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| source | Cambridge University Press Journals Complete |
| subjects | Astronomy Astrophysics Contributed Papers Imaging techniques Magnetic fields Peculiar stars Stars & galaxies Stellar magnetic fields Topology |
| title | Searching for a link between the presence of chemical spots on the surface of HgMn stars and their weak magnetic fields |
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