Abstract
In this paper, the correlations of gamma ray with other bands are discussed for highly polarized blazars. The results show gamma rays are beamed. It is closely associated with the radio band emission, but not associated with optical or X-ray emissions. Gamma ray emission is likely from resynchrotron-self-Compton (SSC) process.
Similar content being viewed by others
References
Bertsch, D.L., et al.: 1993,Astrophys. J. 405 L21.
Biermann, P.I., et al.: 1987,Astron. Astrophys. 185, 9.
Bloom, S.D. and Marscher, A.P.: 1991,Astrophys. J. 366, 16.
Boznyan, E.P. et al.: 1990,Astron. J. 99, 1421.
Bregman, J.N.,et al.: 1987, in: Y. Konds (ed.),Sci. Accomplishments of the IUE, D. Reidel Publ. Co., p. 685.
Bregman, J.N., et al.: 1985,Astrophys. J. 291, 505.
Brinkmann, W., et al.: 1994,Astron. Astrophys. 281, 355.
Brown, I.M.J., et al.: 1989,Astrophys. J. 340 129.
Dermer, C.D., et al.: 1992,Mon. Not. R. Astron. Soc. 256, L27.
Dondi, L. and Ghisellini, G.: 1995,Mon. Not. R. Astron. Soc. 273, 583.
Fan, J.H.: 1996,Astrophys. Lett. Commun. (in press).
Fan, J.H., et al.: 1996,Astron. Astrophys. Suppl. 116, 409.
Fichter, C.E.: 1994,Astrophys. J. Suppl. 90, 917.
Fichtel, C.E., et al.: 1994,Astrophys. J., Suppl. 434, 557.
Fichtel, C.E.,et al.: 1992,EGRET Contri. to The Compton Obser. Symp., Washington Uni. MO., Oct. 15–17.
Gear, W.K., et al.: 1994,Mon. Not. R. Astron. Soc. 267, 167.
Ghisellini, G., et al.: 1993,Astrophys. J. 407, 65.
Ghisellini, G., et al.: 1986,Astrophys. J. 310, 317.
Giovanoni, P.M. and Kazans, D.: 1990,Nature 345, 319.
Hartman, R.C., et al.: 1993,Astrophys. J. 407, L41.
Hartman, R.C., et al.: 1992,Astrophys. J. 385, L1.
Hunter, S.D., et al.: 1993,Astrophys. J. 409, 134.
Impey, C.D. and Tapia, S.: 1990,Astrophys. J. 354, 124.
Impey, C.D. and Tapia, S.: 1988,Astrophys. J. 333, 666.
Kazans, D.: 1991, in: S.S. Holt, S.G. Neff and C. Murry (eds.),The AGN Paradygm Workshop, AIP Conf. Proc. 254), 301.
Kniffen, D.A., et al.: 1993,Astrophys. J. 411, 133.
Kuhr, H., et al.: 1981,Astron. Astrophys. Suppl. 45, 367.
Ledden, J. and O'Dell, S.L.: 1985,Astrophys. J. 298, 630.
Makino, K.,et al.: 1992, in:International Symp. on Neutrino Astrophys., Takayama, Kamioka, Japan, Oct. 19–22.
Makino, K.: 1989,Proc. 23rd ESLAB Symp., ESA SP-296, p. 803.
Marscher, A.P. and Bloom, S.D.: 1991, in: S. Shrader, N. Gehrels and B. Dennis (eds.),The Compton Obser. Sci. Workshop, NASA Conf. Publ., p. 346.
Mathematics Institute, Chinese Academy of Sciences: 1972,Method for Statistics, Scientific Press of China, p. 100–110.
Mattox, J.R., et al.: 1993,Astrophys. J.,410, 609.
Maraschi, L., et al.: 1986,Astrophys. J.,310, 325.
Nolan, P.L., et al.: 1993,Astrophys. J. 414, 82.
Padovani, P.,et al.: 1993,Mon. Not. R. Astron. Soc. 263, 461 p.
Perly, R.A.: 1982,Astron. J. 87, 859.
Pian, E.,et al.: 1994, Submitted toAstrophys. J.
Sambrunna, R.M.,et al.: 1994,Astrophys. J. (in press).
Schachter, J. and Elvis, M.: 1993,Astrophys. J. Suppl. 92, 623.
Stickel, M., et al.: 1991,Astrophys. J. 374, 431.
Swanenburg, B.N., et al.: 1978,Nature 275, 298.
Thompson, D.J., et al.: 1993,Astrophys. J. 415, L13.
Thompson, D.J.,et al.: 1993,IAU Symp. 159 (in press).
Treves, A., et al.: 1993,Astrophys. J. 406, 447.
Veron-cetty, M.P. and Veron, P.: 1991,ESO Sci. Report, N7.
von Montigny, C., et al.: 1995,Astrophys. J. 440, 525.
von Montigny, C., et al.: 1993, in: N. Gehrels and M., Friedlander (eds.),Compton Gamma Ray Obser., American Institute of Phys., New York, p. 518.
Wall, J.V. and Peacock, J.A.: 1985,Mon. Not. R. Astron. Soc. 216, 173.
Wilkes, B.J., et al.: 1994,Astrophys. J. Suppl. 92, 53.
Worrall, D.M. and Wilkes, B.J.: 1990,Astrophys. J. 360, 396.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Fan, J.H. Gamma-ray emission of blazars. Astrophys Space Sci 246, 119–128 (1996). https://doi.org/10.1007/BF00637403
Received:
Accepted:
Issue Date:
DOI: https://doi.org/10.1007/BF00637403