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Observational Studies of Cataclysmic Variable Evolution: Of Samples, Biases and Surprises

Published online by Cambridge University Press:  22 February 2018

B.T. Gänsicke
B.T. Gänsicke*
Affiliation:
Department of Physics, University of Warwick, Coventry CV4 7AL, UK

Abstract

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I present, brief status reports on three large observational projects that are designed to test our current understanding of the evolution of cataclysmic variables (CVs): The spectroscopic selection of new CVs in the Hamburg Quasar Survey, the search for pre-CVs based on Sloan colours and UK Schmidt/6dF multiobject spectroscopy, and the identification of CVs that descended from supersoft X-ray binaries using a HST/STIS far-ultraviolet spectroscopic survey.

Resumen

Resumen

Presento un breve informe sobre el estado de tres grandes proyoctos observacionales destinados a verificar nuestra actual comprensión de la evolucion de variables cataclísmicas (CVs): la selección espectroscópica de las nuevas CVs en el Hamburg Quasar Survey, la búsqueda de pre-CVs basándose en los colores de Sloan y en la espectroscopía multi-objeto UK Schmidt/6dF y la identificación de CVs que proceden de binarias de rayos X supersuaves, utilizando el “survey” espectroscópico en el ultravioleta lejano del HST/STIS.

Keywords

NovaeCataclysmic Variables — StarsEvolution
Type
The Contributed Papers
Information
International Astronomical Union Colloquium , Volume 194: Compact binaries in the galaxy and beyond , 2004 , pp. 152 - 154
Copyright
Copyright © Instituto de astronomia/revista mexicana de astronomίa y astrofίsica 2004

References

Abazajian, K., Adelman-McCarthy, J. K., Agüeros, M. A., et al. 2003, 126, 2081 Google Scholar
Andronov, N., Pinsonneault, M. & Sills, A. 2003, ApJ, 582, 358 Google Scholar
Araujo-Betancor, S., Gänsicke, B. Т., Hagen, H.-J., et al. 2004, this volumeGoogle Scholar
Downes, R. A.. Webbink, R. F., Shara, M. M., et al. 2001, PASP, 113, 764 Google Scholar
Gänsicke, B. T., Hagen, H.-J. & Engels, D. 2002, ASP Conf. Ser. 261, 190 Google Scholar
Gänsicke, B. T., Szkody, P., de Martino, D., et al. 2003, Ap.J, 594, 443 Google Scholar
Gänsicke, B. Т., Araujo-Betancor, S., Hagen, H.-J., et al. 2004, this volumeGoogle Scholar
Hagen, H.-J., Groote, D., Engels, D. & Reimers, D. 1995, A&rAS, 111, 195 Google Scholar
King, A. R. 1988, QJRAS, 29, 1 Google Scholar
King, A. R. & Schenker, K. 2002, ASP Conf. Ser. 261, 233 Google Scholar
Langer, N., Deutschmann, A., Wellstein, S., & Hö;flich, P. 2000, A&A, 362, 1046 Google Scholar
Raymond, S. N., Szkody, P., Hawley, S. L., et al. 2003, AJ. 125, 2621 CrossRefGoogle Scholar
Rodríguez-Gil, P., Gänsicke, B. Т., Hagen, H.-J., et al. 2004. A&A submittedGoogle Scholar
Schenker, K. & King, A. R. 2002, ASP Conf. Ser. 261, 242–251 Google Scholar
Schenker, K.. King, A. R.. Kolb, U., et al. 2002, MNRAS, 337, 1105 Google Scholar
Schreiber, M. R. & Gänsicke, B. Т. 2003. A&A, 406, 305 Google Scholar
Spruit, H. C. & Taam, R. E. 2001. ApJ, 548, 900 Google Scholar