Autor: |
Aurière, M., Wade, G. A., Silvester, J., Lignières, F., Bagnulo, S., Bale, K., Dintrans, B., Donati, J. F., Folsom, C. P., Gruberbauer, M., Hui Bon Hoa, A., Jeffers, S., Johnson, N., Landstreet, J. D., Lèbre, A., Lueftinger, T., Marsden, S., Mouillet, D., Naseri, S., Paletou, F., Petit, P., Power, J., Rincon, F., Strasser, S., Toqué, N., Aurière, M., Wade, G. A., Silvester, J., Lignières, F., Bagnulo, S., Bale, K., Dintrans, B., Donati, J. F., Folsom, C. P., Gruberbauer, M., Hui Bon Hoa, A., Jeffers, S., Johnson, N., Landstreet, J. D., Lèbre, A., Lueftinger, T., Marsden, S., Mouillet, D., Naseri, S., Paletou, F., Petit, P., Power, J., Rincon, F., Strasser, S., Toqué, N. |
Zdroj: |
Astronomy and Astrophysics; December 2007, Vol. 475 Issue: 3 p1053-1065, 13p |
Abstrakt: |
Aims.We investigated a sample of 28 well-known spectroscopically-identified magnetic Ap/Bp stars, with weak, poorly-determined or previously undetected magnetic fields. The aim of this study is to explore the weak part of the magnetic field distribution of Ap/Bp stars. |
Databáze: |
Supplemental Index |
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