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Searching for weak or complex magnetic fields in polarized spectra of Rigel

Published online by Cambridge University Press:  12 July 2011

Matthew Shultz
Affiliation:
Queen's University, Canada Royal Military College, Canada
Gregg A. Wade
Affiliation:
Royal Military College, Canada
Coralie Neiner
Affiliation:
Paris-Meudon Observatory
Nadine Manset
Affiliation:
Canada-France-Hawaii Telescope Corporation
Véronique Petit
Affiliation:
Royal Military College, Canada West Chester U
Jason H. Grunhut
Affiliation:
Queen's University, Canada Royal Military College, Canada
Edward Guinan
Affiliation:
Villanova U
David A. Hanes
Affiliation:
Queen's University, Canada
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Abstract

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Seventy-eight high-resolution Stokes V, Q and U spectra of the B8Iae supergiant Rigel were obtained with the ESPaDOnS spectropolarimeter at CFHT and its clone NARVAL at TBL in the context of the Magnetism in Massive Stars (MiMeS) Large Program, in order to scrutinize this core-collapse supernova progenitor for evidence of weak and/or complex magnetic fields. In this paper we describe the reduction and analysis of the data, the constraints obtained on any photospheric magnetic field, and the variability of photospheric and wind lines.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2011

References

Abbott, D. C., Bieging, J. H., Churchwell, E., & Cassinelli, J. P. 1980, ApJ, 238, 196Google Scholar
Aufdenberg, J. P., Ludwig, H.-G., Kervella, P., Mérand, A. et al. 2008, in: Richichi, A., Delplancke, F., Paresce, F., & Chelli, A. (eds.), The Power of Optical/IR Interferometry: Recent Scientific Results and 2nd Generation, ESO Astrophysics Symposia, p. 71Google Scholar
Barlow, M. J. & Cohen, M. 1977, ApJ, 213, 737Google Scholar
Bates, B., Giaretta, D. L., McCartney, D. J., McQuoid, J. A. et al. 1980, MNRAS, 190, 611Google Scholar
Cantiello, M., Langer, N., Brott, I., de Koter, A. et al. 2009, A&A, 499, 279Google Scholar
Israelian, G., Chentsov, E., & Musaev, F. 1997, MNRAS, 290, 521Google Scholar
Kaufer, A., Stahl, O., Wolf, B., Gaeng, T. et al. 1996a, A&A, 305, 887Google Scholar
Kaufer, A., Stahl, O., Wolf, B., Gaeng, T. et al. 1996b, A&A, 314, 599Google Scholar
Kaufer, A., Stahl, O., Wolf, B., Fullerton, A. W. et al. 1997, A&A, 320, 273Google Scholar
Puls, J., Vink, J. S., & Najarro, F. 2008, A&AR, 16, 209Google Scholar
Przybilla, N., Butler, K., Becker, S. R., & Kudritzki, R. P. 2006, A&A, 445, 1099Google Scholar
Sanford, R. F. 1947, ApJ, 105, 222Google Scholar
ud-Doula, A. & Owocki, S. P. 2002, ApJ, 576, 413Google Scholar