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- W2132908727 abstract "We report the discovery of a medium-strength (∼0.5 kG) magnetic field on the young, massive star τ Sco (B0.2 V), which becomes the third-hottest magnetic star known. Circularly polarized Zeeman signatures are clearly detected in observations collected mostly with the ESPaDOnS spectropolarimeter, recently installed on the 3.6-m Canada–France–Hawaii Telescope; temporal variability is also clearly established in the polarimetry, and can be unambiguously attributed to rotational modulation with a period close to 41 d. Archival ultraviolet (UV) spectra confirm that this modulation repeats over time-scales of decades, and refine the rotation period to 41.033 ± 0.002 d." @default.
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- W2132908727 date "2006-08-01" @default.
- W2132908727 modified "2023-10-06" @default.
- W2132908727 title "The surprising magnetic topology of Sco: fossil remnant or dynamo output?" @default.
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- W2132908727 doi "https://doi.org/10.1111/j.1365-2966.2006.10558.x" @default.
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