Abstract
SS Cyg is the brightest known and therefore best studied classical dwarf nova and it was the first one from which X-ray radiation was discovered. SS Cyg is unique because it has been detected at very wide range of energies, from a few eV up to ⋃ 10 keV (Jones & Watson 1992). It was chosen as the first cataclysmic variable for X-ray observations with the Japanese satellite ASCA. Simultaneous optical photometric and spectroscopic observations were also provided for completeness of the study.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
References
Howarth, I.D., 1978, J.British Astron.Assoc., 88, 458
Jones, M.H., Watson, M.G., 1992, MNRAS, 257, 633
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1996 Kluwer Academic Publishers
About this paper
Cite this paper
Voloshina, I. (1996). Results of Optical Monitoring of the Dwarf Nova SS Cyg During the 1993 Campaign of Coordinated Observations with the Asca Satellite. 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_21
Download citation
DOI: https://doi.org/10.1007/978-94-009-0325-8_21
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-6632-7
Online ISBN: 978-94-009-0325-8
eBook Packages: Springer Book Archive