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Autor:
Wade, G. A., Neiner, C., Alecian, E., Grunhunt, H. H., Petit, V., Batz, B., Bohlender, D. A., Cohen, D. H., Henrichs, H. F., Kochukhov, O., Landstreet, J. D., Manset, N., Martins, F., Mathis, S., Oksala, M. E., Owocki, S. P., Rivinius, Th., Schultz, M. E., Sundqvist, J. O., Townsend, R. H.D., Doula, A., Bouret, J. C., Braithwaite, J., Briquet, M., Carciofi, A. C., David-Uraz, A., Folsom, C. P., Fullerton, A. W., Leroy, B., Marcolino, W. L.F., Moffat, A. F.J., Naze, Y., St Louis, N., Auriere, M., Bagnulo, S., Bailey, J. D., Barba, R. H., Blazere, A., Bohm, T., Catala, C., Donati, J-F, Ferrario, L., Harrington, D., Howarth, I. D., Ignace, Richard, Kaper, L., Luftinger, T., Prinja, R., Vink, J. S., Weiss, W. W., Yakunin, I.
Publikováno v:
ETSU Faculty Works.
The MiMeS (Magnetism in Massive Stars) project is a large-scale, high-resolution, sensitive spectropolarimetric investigation of the magnetic properties of O- and early B-type stars. Initiated in 2008 and completed in 2013, the project was supported