Abstract
The estimation of some important parameters of pulsars is discussed. The results have been compared with the RS model and applied to the estimation of radio luminosity and the beaming factor.
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References
Manchester, M. N. and Taylor, J. H.: 1977,Pulsars, pp. 217 and 224.
Jones, P. B.: 1977,Monthly Notices Roy. Astron. Soc. 178, 187.
Proszynski, M.: 1978,Astron. Astrophys. 79, 8.
Wu Xinji et al.: 1982,Chinese Astron. Astrophys. 6, 216.
Narayan, R. and Vivekanand, M.: 1982,Astron. Astrophys. 113, L3.
Ruderman, M. A. and Sutherland, P. G.: 1975,Astrophys. J. 196, 51.
Taylor, J. H. and Manchester, R. N.: 1975,Astron. J. 80, 794.
Gunn, J. E. and Ostriker, J. D.: 1970,Astrophys. J. 160, 979.
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Xinji, W., Guojun, Q., Xiaoyang, X. et al. Estimation of some parameters of pulsars and their applications. Astrophys Space Sci 119, 101–104 (1986). https://doi.org/10.1007/BF00648823
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DOI: https://doi.org/10.1007/BF00648823