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Spectral Properties of the X-Ray Objects GX 3 + 1, GX 354–5 and Sco XR-1

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A Corrigendum to this article was published on 30 November 1968

Abstract

The spectra of three X-ray objects have been measured from a balloon, and suggest that the sources are supernova remnants, and that the X-ray emission is due to magnetic bremsstrahlung.

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References

  1. Peterson, L. E., Jerde, R. L., and Jacobson, A. S., AIAA Journal, 5, 1921 (1967).

    Article  ADS  Google Scholar 

  2. Boldt, E., McDonald, F. B., Riegler, G., and Serlemitsos, P., Phys. Rev. Lett., 17, 447 (1966).

    Article  ADS  Google Scholar 

  3. Friedman, H., Byram, E. T., and Chubb, T. A., Science, 156, 374 (1967).

    Article  ADS  CAS  Google Scholar 

  4. Bradt, H., Naranan, S., and Spada, G., Ap. J. (in the press).

  5. Gursky, H., Gorenstein, P., and Giacconi, R., Ap. J., 150, L75 (1967).

    Article  ADS  Google Scholar 

  6. Peterson, L. E., Jacobson, A. S., Pelling, R. M., and Schwartz, D. A., Proc. Tenth Intern. Conf. Cosmic Rays, Calgary (1968).

  7. Peterson, L. E., and Jacobson, A. S., Ap. J., 145, 962 (1966).

    Article  ADS  CAS  Google Scholar 

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BUSELLI, G., CLANCY, M., DAVISON, P. et al. Spectral Properties of the X-Ray Objects GX 3 + 1, GX 354–5 and Sco XR-1. Nature 219, 1124–1127 (1968). https://doi.org/10.1038/2191124a0

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