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The Continuum Energy Distribution of the Old-Nova GK Per (1901)
release_lmst7hsfzrhajcnp42uf3biusq
by
A. Bianchini,
F. Sabbadin
Published
in International Astronomical Union Colloquium
by Cambridge University Press (CUP).
1983 Volume 72, p127-131
Abstract
<jats:title>ABSTRACT</jats:title>The observed X-ray to IR continuum energy distribution of the old-nova GK Per, corrected for the contribution of the late-type secondary and for i.s. extinction,is found to be consistent with the model of an accreting magnetic white dwarf. Furthermore, we discuss plausible modifications of the standard disc structure caused by the presence of magnetic field lines threading the disc and evaluate the contribution to the observed radiation field from several physical mechanisms.
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