- Bagnulo, S., Landolfi, M., & Landi Degl'Innocenti, M. 1996, A&A, 308, 115 [NASA ADS] [Google Scholar]
- Bagnulo, S. 2002, private communication [Google Scholar]
- Bagnulo, S., Landi Degl'Innocenti, M., Landolfi, M., & Mathys, G. 2002, A&A, 394, 1023 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
- Budaj, J. 1999, MNRAS, 310, 419 [NASA ADS] [CrossRef] [Google Scholar]
- Didelon, P. 1987, The Messenger, 49, 5 [NASA ADS] [Google Scholar]
- Donati, J.-F., Semel, M., Carter, B. D., Rees, D. E., & Cameron, A. C. 1997, MNRAS, 291, 658 [NASA ADS] [CrossRef] [MathSciNet] [Google Scholar]
- Donati, J.-F., Collier Cameron, A., Hussain, G. A. J., & Semel, M. 1999, MNRAS, 302, 437 [NASA ADS] [CrossRef] [Google Scholar]
- ESA 1997, The Hipparcos and Tycho Catalogues, ESA Sp-1200 [Google Scholar]
- Gerth, E., Glagolevskij, Yu. V., & Sholz, G. 1997, in Stellar Magnetic Fields, ed. Yu. V. Glagolevskij, & I. I. Romanyuk (Moscow), 67 [Google Scholar]
- Glagolevskij, Yu. V., & Chountonov, G. A. 1998, Bull Spec. Astrophys. Obs., 45, 105 [NASA ADS] [Google Scholar]
- Glagolevskij, Yu. V., & Gerth, E. 2002, A&A, 382, 935 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
- Hensberge, H. 1993, Long term variability in CP stars, in Peculiar versus normal phenomena in A-type and related stars, IAU Colloq. 138, ed. M. M. Dworetsky, F. Castelli, & R. Faraggiana, Astron. Soc. Pac. Conf. Ser., 44, 547 [Google Scholar]
- Hubrig, S., North, P., & Mathys, G. 2000, ApJ, 539, 352 [NASA ADS] [CrossRef] [Google Scholar]
- Khalack, V. R., Khalack, Yu. N., Shavrina, A. V., & Polosukhina, N. S. 2001a, AZh, 78, N7, 655 [Google Scholar]
- Khalack, V. R., Khalack, Yu. N., Shavrina, A. V., & Polosukhina, N. S. 2001b, in Magnetic Fields Across the Hertzsprung-Russel Diagram, ed. G. Mathys, S. K. Solanki, & D. T. Wickramasinghe (San Francisco: ASP), 329 [Google Scholar]
- Khalack, V. R. 2002, A&A, 385, 986 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
- Landau, L. D., & Lifshits, E. M. 1988, The classical Theory of Fields, vol. 2, 7th edition (Moscow), 510 [Google Scholar]
- Landstreet, J. D., & Mathys, G. 2000, A&A, 359, 213 [NASA ADS] [Google Scholar]
- Leeman, S. 1964, Mon. Not. Astr. Soc. South Africa, 23, 6 [NASA ADS] [Google Scholar]
- Nelder, A. J., & Mead, R. 1965, Computer Journal, 7, 308 [CrossRef] [Google Scholar]
- Martinez, P., & Kurtz, D. W. 1994, MNRAS, 271, 129 [NASA ADS] [CrossRef] [Google Scholar]
- Mathys, G. 1991, A&AS, 89, 121 [NASA ADS] [Google Scholar]
- Mathys, G. 1995a, A&A, 293, 733 [NASA ADS] [Google Scholar]
- Mathys, G. 1995b, A&A, 293, 746 [NASA ADS] [Google Scholar]
- Mathys, G., & Hubrig, S. 1997, A&AS, 124, 475 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
- Mathys, G., Hubrig, S., Landstreet, J. D., Lanz, T., & Manfroid, J. 1997, A&AS, 123, 353 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
- Moss, D. 2001, in Magnetic Fields Across the Hertzsprung-Russel Diagram, ed. G. Mathys, S. K. Solanki, & D. T. Wickramasinghe (San Francisco: ASP), 305 [Google Scholar]
- Press, W. H., Teukolsky, S. A., Vetterling, W. T., & Flannery, B. P. 1992, Numerical recipes in C: the art of scientific computing, 2nd ed. (Cambridge University Press), 995 [Google Scholar]
- Pyper, D. M., Ryabchikova, T., Malanushenko, V., et al. 1998, A&A, 339, 822 [NASA ADS] [Google Scholar]
- Schaller, G., Schaerer, D., Meynet, G., & Maeder, A. 1992, A&AS, 96, 269 [Google Scholar]
- Strasser, S., Landstreet, J. D., & Mathys, G. 2001, A&A, 378, 153 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
Free Access
| Issue |
A&A
Volume 403, Number 1, May III 2003
|
|
|---|---|---|
| Page(s) | 179 - 185 | |
| Section | Stellar structure and evolution | |
| DOI | https://doi.org/10.1051/0004-6361:20030322 | |
| Published online | 29 April 2003 | |
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.