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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Peterson, L. E., Jerde, R. L., and Jacobson, A. S., AIAA Journal, 5, 1921 (1967).
Boldt, E., McDonald, F. B., Riegler, G., and Serlemitsos, P., Phys. Rev. Lett., 17, 447 (1966).
Friedman, H., Byram, E. T., and Chubb, T. A., Science, 156, 374 (1967).
Bradt, H., Naranan, S., and Spada, G., Ap. J. (in the press).
Gursky, H., Gorenstein, P., and Giacconi, R., Ap. J., 150, L75 (1967).
Peterson, L. E., Jacobson, A. S., Pelling, R. M., and Schwartz, D. A., Proc. Tenth Intern. Conf. Cosmic Rays, Calgary (1968).
Peterson, L. E., and Jacobson, A. S., Ap. J., 145, 962 (1966).
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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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DOI: https://doi.org/10.1038/2191124a0
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