磁星
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摘要: 脉冲星通常具有很强的表面磁场,是地球平均磁场强度的万亿倍,可达1012高斯。超强磁场脉冲星(简称为磁星或磁陀星)表面磁场强度比一般脉冲星还要高出两个数量级,可谓是脉冲星家族中磁能天花板。
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① Duncan, R. C. & Thompson, C., 1992, ApJL, 392, L9
② Kaspi, V. M. & Beloborodov, A. M., 2017, ARA&A, 55, 261-301
③ Mazets, E. P., Golentskii, S. V., Ilinskii, V. N. et al. 1979, Nature, 282, 587-589
④ Cline, T. L., Desai, U. D., Teegarden, B. J. et al. 1982, ApJ, 255, L45-L48
⑤ Mazets, E. P., Golenetskij, S. V. & Guryan, Y. A., 1979, SvAL, 5, 343-344
⑥ Kouveliotou, C., Norris, J. P., Cline, T. L. et al. 1987, ApJL, 322, L21
⑦ Laros, J. G., Fenimore, E. E., Klebesadel, R. W et al. 1987, ApJL, 320, L111
⑧ Thompson, C. & Duncan, R. C., 1995, MNRAS, 275, 255-300
⑨ Thompson, C. & Duncan, R. C., 1996, ApJ, 473, 322
⑩ Kouveliotou, C., Dieters, S., Strohmayer, T. et al. 1998, Nature, 393, 235-237
⑪ Kouveliotou, C., Strohmayer, T., Hurley, K. et al. 1999, ApJ, 510, L115-L118
⑫ Gregory, P. C. & Fahlman, G. G., Nature, 287, 805-806
⑬ Gavriil, F. P., Kaspi, V. M. & Woods, P. M., 2002, Nature, 419, 142-144
⑭ Kaspi, V. M., Gavriil, F. P. & Woods, P. M., 2003, ApJ, 588, L93-L96
⑮ Kaspi, V. M., Lackey, J. R. & Chakrabarty, D., 2000, ApJ, 537, L31-L34
⑯ Thompson, C., Lyutikov, M. & Kulkarni, S. R., 2002, ApJ, 574, 332-355
⑰ Beloborodov, A. M., 2009, ApJ, 703, 1044-1060
⑱ Yu, Y.-B. & Huang, Y.-F., 2016, RAA, 16, 75
⑲ Archibald, R. F., Kaspi, V. M., Ng, C.-Y. et al. 2013, Nature, 497, 591-593
⑳ Tong, H., 2014, ApJ, 784, 86
㉑ Hurley, K., Boggs, S. E., Smith, D. M. et al. 2005, Nature, 434, 1098-1103
㉒ Lin, L., Kouveliotou, C., Baring, M. G. et al. 2011, ApJ, 739, 87
㉓ Kaneko, Y., Göğüş, E., Baring, M. G. et al. 2021, ApJ, 916, 7
㉔ Lin, L., Göǧüş, E., Baring, M. G. et al. 2012, ApJ, 756, 54
㉕ Cai, C., Xiong, S.-L., Lin, L. et al. 2022, ApJS, accepted
㉖ Lyubarsky, Y. E., 2002, MNRAS, 332, 199-204
㉗ Rea, N., Esposito, P., Turolla, R. et al. 2010, Science, 6006, 944
㉘ Tiengo, A., Esposito, P., Mereghetti, S. et al. 2013, Nature, 7462, 312-314
㉙ Rodríguez Castillo, G. A., Israel, G. L., Tiengo, A. et al. 2016, MNRAS, 456, 4145-4155
㉚ Tong, H., Xu, R. X., Song, L. M. et al. 2013, ApJ, 768, 144
㉛ Kuiper, L. & Hermsen, W., 2009, A&A, 501, 1031-1046
㉜ Livingstone, M. A., Kaspi, V. M. & Gavriil, F. P., 2010, ApJ, 710, 1710-1717
㉝ Göğüş, E., Lin, L., Kaneko, Y. et al. 2016, ApJL, 829, L25
㉞ Archibald, R. F., Kaspi, V. M., Tendulkar, S. P. et al. 2016, ApJL, 829, L21
㉟ CHIME/FRB Collaboration, 2020, Nature, 587, 54-58
㊱ Bochenek, C. D., Ravi, V., Belov, K. V. et al. 2020, Nature, 587, 59-62
㊲ Li, C. K., Lin, L., Xiong, S. L. et al. 2021, Nature Astronomy, 5, 378-384
㊳ 林琳,葛明玉,李承奎,张冰,2021年2月,《现代物理知识》,33, 41-45 ㊴ Lin, L., Zhang, C. F., Wang, P. et al. 2020, Nature, 587, 63-65
㊵ Roberts, O. J., Veres, P., Baring, M. G. et al. 2021, Nature, 589, 207-210
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