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Confirmation of ξ1 CMa’s ultra-slow rotation: magnetic polarity reversal and a dramatic change in magnetospheric UV emission lines
External Source
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Document Type
Version of Record
Authors
C Erba (Department of Physics and Astronomy, Bartol Research Institute, University of Delaware, Newark, DE 19716, USA)
M E Shultz (Department of Physics and Astronomy, Bartol Research Institute, University of Delaware, Newark, DE 19716, USA)
V Petit (Department of Physics and Astronomy, Bartol Research Institute, University of Delaware, Newark, DE 19716, USA)
A W Fullerton (Space Telescope Science Institute, Baltimore, MD 21218, USA)
H F Henrichs (Anton Pannekoek Institute for Astronomy, University of Amsterdam, Science Park 904, NL-1098 XH Amsterdam, the Netherlands)
O Kochukhov (Department of Physics and Astronomy, Uppsala University, Box 516, SE-751 20 Uppsala, Sweden)
T Rivinius (European Organisation for Astronomical Research in the Southern Hemisphere (ESO), Casilla 19001, Santiago 19, Chile)
G A Wade (Department of Physics and Space Science, Royal Military College of Canada, PO Box 17000, Station Forces, Kingston, ON K7K 0C6, Canada)
Date Acquired
February 8, 2025
Publication Information
Publication: Monthly Notices of the Royal Astronomical Society
Publisher: Oxford University Press (OUP)
Volume: 506
Issue: 2
ISSN: 0035-8711
e-ISSN: 1365-2966
DOI: 10.1093/mnras/stab1454
Funding Number(s)
funding: HST-AR-15794.001-A
funding: NAS 5-26555
Distribution Limits
Public

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