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Long-Term Monitoring of Polars

Published online by Cambridge University Press:  23 April 2012

B. Kalomeni
B. Kalomeni*
Affiliation:
Department of Astronomy and Space Sciences, University of Ege, 35100, İzmir, Turkey Department of Physics, İzmir Institute of Technology, 35430, İzmir, Turkey
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Abstract

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We present long-term observations of magnetic cataclysmic variables AM Her, AN UMa, AR UMa, DP Leo, and V1309 Ori obtained with the ROTSEIIId telescope. All data have been analysed and preliminary results indicate periods of 170 days, 217 days, and 180 days for AM Her, AN UMa, and AR UMa, respectively.

Keywords

cataclysmic variablesstars: individual (AM Her, AN UMa, AR UMa, DP Leo, V1309 Ori
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Symposium S282: From Interacting Binaries to Exoplanets: Essential Modeling Tools , July 2011 , pp. 91 - 92
Copyright
Copyright © International Astronomical Union 2012

References

Beuermann, K. & Thomas, H.-C., 1993, AdSpR, 13, 115Google Scholar
Beuermann, K., Buhlmann, J., Diese, J., Dreizler, S., Hessman, F. V. et al. , 2011, A&A, 526, 53Google Scholar
Biermann, P., Schmidt, G. D., Liebert, J., Tapia, S., et al. , 1985, ApJ, 293, 303CrossRefGoogle Scholar
Bonnet-Bidaud, J. M., Somova, T. A., & Somov, N. N. 1991, A&A, 251L, 27Google Scholar
Garnavich, P. M., Szkody, P., Robb, R. M., Zurek, D. R., & Hoard, D. W., 1994, ApJ, 435L, 141CrossRefGoogle Scholar
Hearn, D. R. & Marshall, F. J. 1979, ApJ, 232L, 21CrossRefGoogle Scholar
Hessman, F. V., Gansicke, B. T., & Mattei, J. A. 2000, A&A, 361, 952Google Scholar
Kafka, S. & Hoard, D. W. 2009, PASP, 121, 1352CrossRefGoogle Scholar
Kalomeni, B., Pekünlü, E. R., & Yakut, K. 2005, Ap&SS, 296, 477Google Scholar
Kalomeni, B. & Yakut, K. 2008, AJ, 136, 2367CrossRefGoogle Scholar
Kalomeni, B. 2011, in preparationGoogle Scholar
Katajainen, S., Piirola, V., Ramsay, G., Scaltriti, F., Lehto, H. J., et al. , 2003, MNRAS, 340, 1CrossRefGoogle Scholar
Szkody, P., Vennes, S., Schmidt, G. D., Wagner, R. M., Fried, R., et al. , 1999, ApJ, 520, 841CrossRefGoogle Scholar
Sanad, M. R. 2010, ApSS, 330, 337Google Scholar
Remillard, R. A., Schachter, J. F., Silber, A. D., & Slane, P. 1994, ApJ, 426, 288CrossRefGoogle Scholar
Richman, H. R., Applegate, J. H., & Patterson, J. 1994, PASP, 106, 1075CrossRefGoogle Scholar
Tapia, S. 1976, BAAS, 8, 511Google Scholar
Wenzel, W. 1993, IBVS, 3890, 1Google Scholar
Warner, B. 1988, Nature, 336, 129CrossRefGoogle Scholar
Wu, K. & Kiss, L. L. 2008, A&A, 481, 433Google Scholar