Abstract
Gamma-ray production by particles escaping from a pulsar into the surrounding nebula is considered. The gamma-ray emission decreases with time and such pulsar-nebula complexes will be observed as transient sources.
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References
Bahcall, J. N., Rees, M. J. and Salpeter, E. E.Ap. J., 1970,162, 737.
Gold, T...Nature, 1969,221, 25.
Trimble, V. and Woltjer, L.Ap. J., 1971,163, 197.
Shlovsky, I. S...Supernovae, Wiley, Interscience Publication, New York, 1968.
Ogelman, H. B., Delvaille, J. P. and Greisen, K.Phys. Rev. Lett., 1956,56, 16, 491.
Duthie, J. G., Cobb, R. and Stewart, J.Phys. Rev. Lett., 1966,17, 263.
Frye, G. M., Staib, J. A., Zych, A. D., Hopper, V. D., Rawlinson, W. R. and Thomas, J. A.Nature, 1969,223, 1320.
Fazio, G. G., Helmken, H. F., Rieke, G. H. and Weeks, T. C.Acta Physica Hungaricae, 1970,29 (Suppl. 1), 115.
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Communicated by Prof. R. R. Daniel,f.a.sc.
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Apparao, K.M.V., Rengarajan, T.N. Transient gamma-ray sources. Proc. Indian Acad. Sci. 73, 257–260 (1971). https://doi.org/10.1007/BF03047117
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DOI: https://doi.org/10.1007/BF03047117