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The Solution of the X-Ray Heating Light Curve for 4U2129+47/V1727 Cyg

Published online by Cambridge University Press:  12 April 2016

K. Pavlovski
K. Pavlovski*
Affiliation:
Hvar Observatory, Faculty of Geodesy, Zagreb, Yugoslavia

Abstract

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The X-ray heating light curve of the binary X-ray source 4U2129+47/V1727 Cgy is synthesized. A reliable solution is obtained only after accounting for the influence of an accretion disk. Model parameters achieved by the best fit are discussed. The solution is also discussed in the context of an extended OFF state.

Type
VII. Related Objects
Information
International Astronomical Union Colloquium , Volume 93: Cataclysmic Variables: Recent Multi-Frequency Observations and Theoretical Developments , 1987 , pp. 701 - 705
Copyright
Copyright © Reidel 1987

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