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X-Ray Astronomy in the Exosat Era pp 139–141Cite as

X-Ray Variability of the Am Her Star CW1103+254

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Abstract

The AM Her star CW1103+254 was observed with the low-energy and the medium-energy instruments of EXOSAT on 3 occasions for a total of 10.5 orbital cycles. Both, soft and hard X-rays from CW1103+254 were detected. We report preliminary results on the time variability of the X-ray emission on time scales from 1 minute to 1 month.

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References

  • Beuermann, K., Stella, L., Krautter, J., Proc. Symposium X-ray Astronomy ’84, Bologna, ed. Y. Tanaka, Inst, of Space and Astronaut.Sc., Tokyo (1984)

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  • Larsson, S., private communication (1984)

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  • Schmidt, G.D., Stockman, H.S., Grandi, S.A.,Astrophys.J. 271, 735 (1983)

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  • Stockman, H.S., Foltz, C.B., Schmidt, G.D., Tapia, S.,Astrophys.J. 271 725 (1983)

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Author information

Authors and Affiliations

  1. Institut für Astronomie and Astrophysik, TU Berlin, Germany

    K. Beuermann

  2. MPI für Extraterrestrische Physik, Garching b. München, Germany

    K. Beuermann

  3. ESA, SSD/ESOC, Darmstadt, Germany

    L. Stella

Authors
  1. K. Beuermann
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  2. L. Stella
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Editor information

Editors and Affiliations

  1. Space Science Department of the European Space Agency, ESTEC, The Netherlands

    A. Peacock

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© 1985 D. Reidel Publishing Company

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Cite this paper

Beuermann, K., Stella, L. (1985). X-Ray Variability of the Am Her Star CW1103+254. In: Peacock, A. (eds) X-Ray Astronomy in the Exosat Era. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-5448-9_17

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  • DOI: https://doi.org/10.1007/978-94-009-5448-9_17

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-8906-7

  • Online ISBN: 978-94-009-5448-9

  • eBook Packages: Springer Book Archive

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