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Spectral and intensity variations in cygnus X-3 by the Astronomical Netherlands Satellite

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Abstract

Measurements obtained with the Utrecht (1–8 keV) and Cambridge (1–28 keV) instruments on board the Astronomical Netherlands Satellite are discussed. Particularly, the 4.8 hr period is investigated.

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References

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Authors and Affiliations

  1. Space Research Laboratory, Utrecht, Netherlands

    A. C. Brinkman, J. Heise, R. Mewe, A. J. F. den Boggende, J. Schrijver & E. Gronenschild

  2. Institute of Space and Aeronautical Science, University of Tokyo, Japan

    Y. Tanaka

  3. American Science and Engineering, Cambridge, Mass., USA

    D. R. Parsignault

  4. Smithsonian Astrophysical Observatory, Cambridge, Mass., USA

    J. Grindlay, E. Schreier, H. Schnopper & H. Gursky

Authors
  1. A. C. Brinkman
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  2. J. Heise
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  3. R. Mewe
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  4. A. J. F. den Boggende
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  5. J. Schrijver
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  6. E. Gronenschild
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  7. Y. Tanaka
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  8. D. R. Parsignault
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  9. J. Grindlay
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  10. E. Schreier
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  11. H. Schnopper
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  12. H. Gursky
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Brinkman, A.C., Heise, J., Mewe, R. et al. Spectral and intensity variations in cygnus X-3 by the Astronomical Netherlands Satellite. Astrophys Space Sci 42, 201–204 (1976). https://doi.org/10.1007/BF00645543

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  • DOI: https://doi.org/10.1007/BF00645543

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