Abstract
We report on a 1-day ASCA observation of the eclipsing dwarf nova HT Cas. We confirm the presence of an X-ray eclipse, which is narrow and deep. The data are consistent with the X-rays originating entirely from the immediate neighborhood of the white dwarf. We draw some preliminary conclusions on the boundary layer and other relevant issues.
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Horne, K., Wood, J.H., Steining, R.F., 1991, Ap. J., 378, 271
Ishida, M., 1996, these proceedings, p259
Meyer, F., Meyer-Hofmeister, E., 1994, A&A, 288, 175
van Teeseling, A., 1996, these proceedings, p273
Wood, J.H., Naylor, T., Hassall, B.J.M., Ramseyer, T.F., 1995, MNRAS, 273, 772
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© 1996 Kluwer Academic Publishers
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Mukai, K., Schlegel, E.M., Swank, J.H., Naylor, T., Wood, J.H. (1996). An ASCA observation of the Eclipsing Dwarf Nova HT CAS. 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_79
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DOI: https://doi.org/10.1007/978-94-009-0325-8_79
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-6632-7
Online ISBN: 978-94-009-0325-8
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