Gavin Ramsay, S. B. Potter, David A. H. Buckley, Peter J. Wheatley  Home/Search
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Abstract: CP Tuc (AX J2315--592) shows a dip in X-rays which lasts for approximately half the binary orbit and is deeper in soft X-rays compared with hard X-rays. It has been proposed that this dip is due to the accretion stream obscuring the accretion region from view. If CP Tuc was a polar, as has been suggested, then the length of such a dip would make it unique amongst polars since in those polars in which a dip is seen in hard X-rays the dip lasts for only 0.1 of the orbit. We present optical... (Update)
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BibTeX entry: (Update)
@misc{ ramsay-simultaneous,
author = "Gavin Ramsay and S. B. Potter and David A. H. Buckley and Peter J. Wheatley",
title = "Simultaneous optical polarimetry and X-ray observations of the magnetic
CV CP Tuc (AX J2315-592)",
url = "citeseer.ist.psu.edu/264289.html" }
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