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An X-ray surprise in a magnetic pulsator
Published online by Cambridge University Press: 23 January 2015
Abstract
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ξ1 CMa is a rare β Cep star with a strong magnetic field. To gain new insight on this object, a dedicated campaign using XMM-Newton was performed. These data reveal a new type of variations, X-ray pulsations, posing a new challenge to our understanding of stellar winds.
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- Copyright © International Astronomical Union 2015
References
Oskinova, L. M., Nazé, Y., Todt, H., et al. 2014, Nature Communications 5, 4024CrossRefGoogle Scholar