Elena Mason, Antonio Bianchini, Marina Orio, Robert E. Williams, Koji Mukai, Domitilla de Marino, Timothy . M. C. Abbot, Francesco di Mille
Fast cadence time resolved spectra taken at the CTIO-4m telescope with the RC-spectrograph during 2 consecutive nights revealed a long term modulation of the binary radial velocity. Chandra hard X-ray spectra taken with the HETGS instrument showed features typically observed in magnetic white dwarfs (WD). Here, we present the new data and suggest that CP Pup is possibly a long orbital period intermediate polar.
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http://arxiv.org/abs/1303.2777
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