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The Spin Pulse of the Intermediate Polar V1062 TauriWe combine ASCA and RXTE data of V1062 Tau to confirm the presence of a 62-min X-ray pulsation. We show that the pulsation is caused largely by the variation of dense partial absorption, in keeping with current models of accretion onto magnetic white dwarfs. Further parameterisation of the spin pulse is, however, hampered by ambiguities in the models.
Document ID
20020070806
Acquisition Source
Goddard Space Flight Center
Document Type
Preprint (Draft being sent to journal)
Authors
Hellier, Coel (Keele Univ. United Kingdom)
Beardmore, A. P. (Keele Univ. United Kingdom)
Mukai, Koji (NASA Goddard Space Flight Center Greenbelt, MD United States)
White, Nicholas E.
Date Acquired
September 7, 2013
Publication Date
January 1, 2002
Subject Category
Astrophysics
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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