Abstract
Using the multifrequency radio profiles of pulsar PSR B2319+60, two parameters of inverse Compton scattering model, the initial Lorentz factor and the factor of energy loss of relativistic particles are constrained.
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References
Kijak, J., Gil, J. 1997, Mon. Not. R. Astron. Soc., 288, 631.
Kuz’min, A. D., Xinji, Wu 1992, Astrophys. Space Sci., 190, 209.
Lee, K. J., Cui, X. H., Wang, H. G. et al. 2009, Astrophys. J., 703, 507.
Qiao, G. J. 1988, Vistas Astron., 31, 393.
Qiao, G. J., Liu, J. F., Zhang, B., Han, J. L. 2001, Astron. Astrophys., 377, 964.
Zhang, H., Qiao, G. J., Han, J. L., Lee, K. J., Wang, H. G. 2007, Astron. Astrophys., 465, 525.
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Wang, H.G., Lv, M. Constraint on Parameters of Inverse Compton Scattering Model for PSR B2319+60. J Astrophys Astron 32, 299 (2011). https://doi.org/10.1007/s12036-011-9034-3
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DOI: https://doi.org/10.1007/s12036-011-9034-3