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Temperature Structure of the Disk in V1315 AQL

Published online by Cambridge University Press:  12 April 2016

C. Moreno ,
R. G. M. Rutten  and
V. S. Dhillon
C. Moreno
Affiliation:
Royal Greenwich Observatory, Isaac Newton Group, La Palma, Spain
R. G. M. Rutten
Affiliation:
Royal Greenwich Observatory, Isaac Newton Group, La Palma, Spain
V. S. Dhillon
Affiliation:
Royal Greenwich Observatory, Isaac Newton Group, La Palma, Spain

Abstract

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We present a progress report on the analysis of time-resolved spectrophotometric observations of the cataclysmic variable V1315 Aql. The spectral range of the data covers the entire Balmer series up to and including the Balmer jump. We aim to use these data to test the steady-state accretion disk model.

Type
Non-Magnetic Cataclysmic Variables
Information
International Astronomical Union Colloquium , Volume 158: Cataclysmic Variables and Related Objects , 1996 , pp. 15 - 16
Copyright
Copyright © Kluwer 1996

References

1. Downes, R.A., Mateo, M., Szkody, P., et al., 1986, Ap. J., 301, 240 Google Scholar
2. Rutten, R.G.M., van Paradijs, J., Tingbergen, J., 1992, A&A, 260, 213 Google Scholar
3. Dhillon, V.S., Marsh, T.R., Jones, D.H.P., 1991, MNRAS, 252, 342 Google Scholar