Abstract
Piirola, Hakala & Coyne (1993) modeled the opjtical/IR light curve of RE0751+14 assuming a uniform shock structure and neglecting the hard X-ray emission. In this paper, we model the light curves at optical/IR and hard X-ray wavelengths and include the effects of the shock structure.
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References
Chanmugam, G., Ray, A., 1984, Ap. J., 285, 252
King, A.R., Frank, J., Ritter, H., 1985, MNRAS, 213, 181
Piirola, V., Hakala, P., Coyne, G.V., 1993, Ap. J., 410, L107
Väth, H., Chanmugam, G., Frank, J., 1996, Ap. J., in press
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© 1996 Kluwer Academic Publishers
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Väth, H. (1996). The Magnetic Field of the Intermediate Polar RE0751+14. In: Evans, A., Wood, J.H. (eds) Cataclysmic Variables and Related Objects. Astrophysics and Space Science Library, vol 208. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0325-8_54
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DOI: https://doi.org/10.1007/978-94-009-0325-8_54
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-6632-7
Online ISBN: 978-94-009-0325-8
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