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2021MNRAS.506.2296E - Mon. Not. R. Astron. Soc., 506, 2296-2308 (2021/September-2)
Confirmation of ξ1 CMa's ultra-slow rotation: magnetic polarity reversal and a dramatic change in magnetospheric UV emission lines.
ERBA C., SHULTZ M.E., PETIT V., FULLERTON A.W., HENRICHS H.F., KOCHUKHOV O., RIVINIUS T. and WADE G.A.
Abstract (from CDS):
Abstract Copyright: © 2021 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society
Journal keyword(s): techniques: polarimetric - stars: early-type - stars: individual: x 1 CMa - stars: magnetic field - stars: massive - ultraviolet: stars
Simbad objects: 8
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