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毕业论文参考文献格式
2024-07-02 20:06:43参考文献 学术堂 韩老师致谢
参考文献[1]黄克谅。类星体与活动星系核[M].北京：中国科学技术出版社，2005.1.[2]马力，2005.4,博士论文，中科院云南天文台。[3]Bottcher,M.,1997,PhDthesis,UniversitatBonn.[4]UrryC.M.,PadovaniP.,UnifiedSchemesforRadio-LoudAct
参考文献
[1] 黄克谅。类星体与活动星系核[M].北京：中国科学技术出版社，2005.1.
[2] 马力，2005.4,博士论文，中科院云南天文台。
[3] B¨ottcher, M., 1997, PhD thesis, Universitat Bonn.
[4] Urry C.M., Padovani P., Unified Schemes for Radio-Loud Active Galactic Nuclei[J]. 1995,PASP,107:803.
[5] Antonucci R.R.J.,Ulvestad J.S., Extended radio emission and the nature of blazars[J].1985, ApJ,249:159.
[6] Ulrich M.H., Maraschi L. & Urry C.M., Variability of Active Galactic Nuclei[J]. ARA&A,1997, 35:45.
[7] Miley G K, Miller J S. Relations between the emission spectra and radio structures of quasars[J],1979, ApJ, 228: 55.
[8] Rees,Martin J.Black Hole Models for Active Galactic Nuclei[J].ARA&A, 1984,22:471.
[9] P Wilson A S, Colbert E J M. The Origin of Powerful Radio Sources [J]. 1995, American Astronomical Society, 186:1502.
[10] Maraschi, L., Ghisellini, G., Tanzi, E. G., et al.Spectral properties of Blazars . C . an X-ray Observed Sampal[J]. ApJ., 1986, 310:325.
[11] Fanaroff,B.L.,Riley,J.M.,The morphology of extragalatic radio sources of high and low luminoisity[J], 1974 ,MNRAS, 167:31.
[12] Kollgaard,R.I.,Wardle,J.F.C.,Roberts,D.H.,Gabuzda,D.C.,Radio constrains on the nature of BLLacertae and their parent population[J] , 1992, AJ, 104:1687.
[13] Angel,J.R.P. & Stockman,H.S.Optical and infrared polarization of active extragalactic objects [J].ARA&A,1980,18:321.
[14] Khachikian,E.Y&Weedman,D.W.,An atlas of Seyfert galaxies[J].1974,ApJ,192,551.
[15] Bradley M.P.,An introduction to active galactic nuclei.Cambridge University Press,1997.24.
[16] Meyer F.,Meyer-Hofmeister E.Outbursts in dwarf novae accretion disks [J]. A&A,1984,132:143.
[17] Lainela, M., Takalo, L. O., Sillanp??, A. The 65 Day Period in 3C 66A during Bright State[J].ApJ,1999,521: 561.
[18] Wagner S.J. & Witzd A., Intraday Variability In Quasars and BL Lac Objects[J]. 1995, ARA&A,33:163.
[19] Carini M.T., Miller H.R., Noble J.C., Sadun A.C., The timescales of the optical variability of blazars.Ⅱ-AP Librae[J].1991,AJ,101:1196.
[20] Zhang X., Zhang L., Zhao G., Xie Z.H., Wu L., Zheng Y.G., Optical Monitoring of Three Gamma-Ray-loud BL Lacertae Objects in 1999-2002[J].2004,AJ,128:1929.
[21] Bertaud C., Wlerick G., Veron P., et al.Etude photometrique de BL Lacertae[J]. 1973, A&A,24:357B.[22] Xie, G. Z., Lu, J. F., Wu, J. X., et al. Determination of several parameters of BL Lacertae objects and relativistic beaming[J]. A&A., 1989, 220:89.
[23] Dai B. Z., Xie G. Z, Li K. H., et al. Rapid Optical Variability of Gamma-Ray-loud Blazars[J]. AJ.2001, 122:290.
[24] Abramowicz, M. A., Nobili, L., Are there black holes in quasars[J]. Nature, 1982, 300:506.
[25] Xie G. Z., Lu J. F. & Wu J .X. et al., Determination of several parameters of BL Lacertae objects and relativistic beaming[J]. A&A., 1989, 220:89.
[26] Wagner S.J. & Witzd A., Intraday Variability In Quasars and BL Lac Objects[J]. ARA&A., 1995,33:163.
[27] Dondi L., Ghisellini G., Gamma-ray-loud blazars and beaming[J]. MNRAS., 1995, 273:583.
[28] Fabian A.C.Theories of the nuclei of active galaxies[C]. Proc, R, Soc. London Ser. A. 1979,366:49.
[29] Cavallo G., Rees M.J, A qualitative study of cosmic fireball sand gamma-raybursts[J]. MNRAS.,1978, 183:359.
[30] 谢光中，李开华，鲍梦贤等。6 个 BL Lacertae 天体的短时标光变[J].1985.科学通报，23:47.
[31] Fabian A.C.Theories of the nuclei of active galaxies[C].1979,Proc,R,Soc.London Ser.A.366:49.
[32] Cavallo G., Rees M.J, A qualitative study of cosmic fireball sand gamma-raybursts[J].1978,MNRAS,183:359.
[33] Miller H.R., Carini M.T., Goodrich B.D., Detection of microvariability for BL Lacertae objects[J].1989,Nature,337:627.
[34] 张雄，谢光中，白金明。用 Jurkevich 方法计算 BL Lac 天体光变周期。天体物理学报，1998.7,第 18 卷 3 期。
[35] 张浩晶，张雄，懂富通等。用小波分析法计算 S5 0716+714 光变周期。 [J].天文学报。2009.4 第50 卷 2 期。
[36] JIANG Chang-jin, JIANG Yong. Fast Fourier transform and C procedures. Hefei: University of Science and Technology of China Press, 2004 , 100-18.
[37] Antonucci, R. R .J., Ulvestad, J. S., Extended radio emission and the nature of blazars[J]. ApJ.,1985, 294:158.
[38] 白金明，谢光中。 BL Lac 天体处于高态与低态时的短时标光变的差异及机制研究[J]. 天体物理学报，1999,19（3）：240.
[39] Xie G.Z., Zhang X., Bai J.M. & Xie Z.H., Gamma-Rayand Near-Infraerd Emission form Gamma-Ray-loud Blazars[J].1998,ApJ,508:180.
[40] 樊军辉， G. E. Romero , ?瑞光。3C273 的光学光变周期[J] . 天文学报。 2001, 42（1）：9-15.
[41] Y. G. Zheng , X. Zhang , X. W. Bi , et al. Long-term Optical Spectra Variability of BL LacertaeObject OJ 287 [J] . MNRAS , 2008. 385 : 823-829.
[42] Horiuchi T. . A model of hydromagnetic turbulent viscosity in radiation-pressure-dominateddisks[J]. PASJ , 1990. 42, 661.
[43] 张雄，谢光中，白？明。 用 Jurkevich 方法分析计算 BLLac 天体的光变周期。 天体物学报。1998. 18 , 260.
[44] Foster G. Time Series Analysis by Projection.I.Statistical Properties of Fourier Analysis[J].AJ,1996, 111:541-55.
[45] Stiephane Mallat. A Wavelet Tour of Signal Processing[M].1999, USA:Academic Press 22-101.
[46] D'Arcangelo, F.D., Marscher, A.P., Jorstad, S.G., et al. Rapid Multiwaveband Polarization Variability in the Quasar PKS 0420-014: Optical Emission from the Compact Radio Jet[J], ApJ,2007, 659: L107-110.
[47] Blandford R.D. & Rees M.J., Some comments on radiation mechanisms in Lacertids[M].,Pittsburgh:Pittsburgh Univ. Press,1978,328:310.
[48] Pearson T.J., Zensus J.A., In Superluminal Radio Source[M].1987,Combridge:Combridge Univ.Press,P1.
[49] Perlman, E. S., Stocke, J. T., Wang, Q. D., et al. Soft X-Ray Observations of a Complete Sample of X-Ray-Selected BL lacertae Objects[J]. ApJ., 1996, 456:451.
[50] Antonucci, R. R .J., Ulvestad, J. S., Extended radio emission and the nature of blazars[J]. ApJ.,1985, 294:158.
[51] Keel .W. C., The jet of PKS 0521-36-an aging counterpart of M87?[J]. ApJ., 1986, 302:296.
[52] Stocke, J. T., liebert, J., Cshmids, G., et al. Optical and radio properties of X-ray selected BLLacertae objects[J]. ApJ., 1985, 298:619.
[53] Elvis M. et al., Most supenmassive black holes must be rapidly rotating[J].2002,ApJ, 565, L75.
[54] Ekers, R.D., Wall, J.V., Shaver, P. A., et al. A complete sample of radio galaxies. I-The radoi data[J]. MNRAS., 1989, 236:727.
[55] Sillanp?? A. et al.OJ 287-Binary pair of supermassive black holes [J].ApJ,1988,325: 628.
[56] Xie, G. Z., Zhang x., Bai, J. M., et al. Gamma-Ray and Nera-Infrared Emission from Gamma-ray-loud Blazars[J]. ApJ., 1998, 508:180.
[57] Wagner S.J.,Witzd A.,Intraday Variability In Quasars and BLLac objects[J],ARA&A,1995, 33,163.
[58] Dondi,L.,Ghisellini,G.,Gamma-ray-loud blazars and beaming[J].1995, MNRAS, 273:583.
[59] Storchi-Bergmann T.et al., The ionization cone, obscured nucleus, and gaseous outflow inNGC3281:A prototypical Seyfert II galaxy?[J].1992, ApJ, 396, 45.
[60] Storchi-Bergmann T.et al., The ionization cone, obscured nucleus, and gaseous outflow inNGC3281:A prototypical Seyfert II galaxy?[J].1992, ApJ, 396, 45.
[61] Hurt T.et al., Ultraviolet imaging polarimetry of narrow-line radio galaxies[J].1999,ApJ, 514,579.
[62] Pier E.A. and Krolik J.H., Infrared spectra of obscuring dust tori around active galactic nuclei.I.Calculational method and basic trends[J].1992,ApJ,401,99.
[63] Wilson A.S. & Tsvetanov Z.L, Ionization cones and radio ejects in active galaxies[J]. 1994, AJ,107,1227.
[64] Done C. et al., NGC4945: The brightest Seyfert II galaxy at 100keV[J].1996, ApJ, 463, L63.
[65] Biermann, P. L., Chirvasa, M., Falcke, H., et al. Single and binary Black Holes and their active environment[C], Proceedings of the 7eme Colloquium Cosmolo-gie, 'High Energy Astrophysics from and for Space' Paris, June 2002, Eds. N.Sanchez and H. de Vega, 11503（astro-ph/0211503）。
[66] Blandford R.D. & Rees M.J., Some comments on radiation mechanisms in Lacertids[M].Pittsburgh:Pittsburgh Univ. Press,1978, 328:310.
[67] Pearson T.J., Zensus J.A., In Superluminal Radio Source[M].1987,Combridge:Combridge Univ. Press,P1.
[68] D'Arcangelo, F.D., Marscher, A.P., Jorstad, S.G., et al. Rapid Multiwaveband Polarization Variability in the Quasar PKS 0420-014: Optical Emission from the Compact Radio Jet[J], ApJ,2007, 659: L107-110.
[69] Urry C.M. & Padovani P., Unified Schemes for Radio-Loud Active Galactic Nuclei[J].1995,PASP,107:803.
[70] Marscher, A.P., Jorstad, S.G., D'Arcangelo, F.D., et al. The inner jet of an active galactic nucleus as revealed by a radio-to-γ-ray outburst[J], Nature, 2008,452: 966-969.
[71] Hartman R.C., B?ttcher M., Aldering G.et al., Multiwavelength Spectra and Models for Blazar 3C 279[J].2001,ApJ,553:683.
[72] Xie G.Z., Lu J.F. & Wu J.X.et al., Determination of several parameters of BL Lacertae objects and relativistic beaming[J].1989,A&A,220:89.
[73] Sikora M., Begelman M.C., Rees M.J., Comptonization of diffuse ambient radiation by a
relativistic jet:The source of gamma rays from blazars?[J].1994,ApJ,421:153.
[74] Chiaberge,Marco.,Ghisellini,Gabriele.,Rapid variability in the synchrotron self-Compton model for blazars [J], 1999, MNRAS, 306: 551.
[75] Dermer C.D., Schlickeiser R., Model for the High-Energy Emission from Blazars[J]. 1993, ApJ,416:458.
[1] 黄克谅。类星体与活动星系核[M].北京：中国科学技术出版社，2005.1.
[2] 马力，2005.4,博士论文，中科院云南天文台。
[3] B¨ottcher, M., 1997, PhD thesis, Universitat Bonn.
[4] Urry C.M., Padovani P., Unified Schemes for Radio-Loud Active Galactic Nuclei[J]. 1995,PASP,107:803.
[5] Antonucci R.R.J.,Ulvestad J.S., Extended radio emission and the nature of blazars[J].1985, ApJ,249:159.
[6] Ulrich M.H., Maraschi L. & Urry C.M., Variability of Active Galactic Nuclei[J]. ARA&A,1997, 35:45.
[7] Miley G K, Miller J S. Relations between the emission spectra and radio structures of quasars[J],1979, ApJ, 228: 55.
[8] Rees,Martin J.Black Hole Models for Active Galactic Nuclei[J].ARA&A, 1984,22:471.
[9] P Wilson A S, Colbert E J M. The Origin of Powerful Radio Sources [J]. 1995, American Astronomical Society, 186:1502.
[10] Maraschi, L., Ghisellini, G., Tanzi, E. G., et al.Spectral properties of Blazars . C . an X-ray Observed Sampal[J]. ApJ., 1986, 310:325.
[11] Fanaroff,B.L.,Riley,J.M.,The morphology of extragalatic radio sources of high and low luminoisity[J], 1974 ,MNRAS, 167:31.
[12] Kollgaard,R.I.,Wardle,J.F.C.,Roberts,D.H.,Gabuzda,D.C.,Radio constrains on the nature of BLLacertae and their parent population[J] , 1992, AJ, 104:1687.
[13] Angel,J.R.P. & Stockman,H.S.Optical and infrared polarization of active extragalactic objects [J].ARA&A,1980,18:321.
[14] Khachikian,E.Y&Weedman,D.W.,An atlas of Seyfert galaxies[J].1974,ApJ,192,551.
[15] Bradley M.P.,An introduction to active galactic nuclei.Cambridge University Press,1997.24.
[16] Meyer F.,Meyer-Hofmeister E.Outbursts in dwarf novae accretion disks [J]. A&A,1984,132:143.
[17] Lainela, M., Takalo, L. O., Sillanp??, A. The 65 Day Period in 3C 66A during Bright State[J].ApJ,1999,521: 561.
[18] Wagner S.J. & Witzd A., Intraday Variability In Quasars and BL Lac Objects[J]. 1995, ARA&A,33:163.
[19] Carini M.T., Miller H.R., Noble J.C., Sadun A.C., The timescales of the optical variability of blazars.Ⅱ-AP Librae[J].1991,AJ,101:1196.
[20] Zhang X., Zhang L., Zhao G., Xie Z.H., Wu L., Zheng Y.G., Optical Monitoring of Three Gamma-Ray-loud BL Lacertae Objects in 1999-2002[J].2004,AJ,128:1929.
[21] Bertaud C., Wlerick G., Veron P., et al.Etude photometrique de BL Lacertae[J]. 1973, A&A,24:357B.[22] Xie, G. Z., Lu, J. F., Wu, J. X., et al. Determination of several parameters of BL Lacertae objects and relativistic beaming[J]. A&A., 1989, 220:89.
[23] Dai B. Z., Xie G. Z, Li K. H., et al. Rapid Optical Variability of Gamma-Ray-loud Blazars[J]. AJ.2001, 122:290.
[24] Abramowicz, M. A., Nobili, L., Are there black holes in quasars[J]. Nature, 1982, 300:506.
[25] Xie G. Z., Lu J. F. & Wu J .X. et al., Determination of several parameters of BL Lacertae objects and relativistic beaming[J]. A&A., 1989, 220:89.
[26] Wagner S.J. & Witzd A., Intraday Variability In Quasars and BL Lac Objects[J]. ARA&A., 1995,33:163.
[27] Dondi L., Ghisellini G., Gamma-ray-loud blazars and beaming[J]. MNRAS., 1995, 273:583.
[28] Fabian A.C.Theories of the nuclei of active galaxies[C]. Proc, R, Soc. London Ser. A. 1979,366:49.
[29] Cavallo G., Rees M.J, A qualitative study of cosmic fireball sand gamma-raybursts[J]. MNRAS.,1978, 183:359.
[30] 谢光中，李开华，鲍梦贤等。6 个 BL Lacertae 天体的短时标光变[J].1985.科学通报，23:47.
[31] Fabian A.C.Theories of the nuclei of active galaxies[C].1979,Proc,R,Soc.London Ser.A.366:49.
[32] Cavallo G., Rees M.J, A qualitative study of cosmic fireball sand gamma-raybursts[J].1978,MNRAS,183:359.
[33] Miller H.R., Carini M.T., Goodrich B.D., Detection of microvariability for BL Lacertae objects[J].1989,Nature,337:627.
[34] 张雄，谢光中，白金明。用 Jurkevich 方法计算 BL Lac 天体光变周期。天体物理学报，1998.7,第 18 卷 3 期。
[35] 张浩晶，张雄，懂富通等。用小波分析法计算 S5 0716+714 光变周期。 [J].天文学报。2009.4 第50 卷 2 期。
[36] JIANG Chang-jin, JIANG Yong. Fast Fourier transform and C procedures. Hefei: University of Science and Technology of China Press, 2004 , 100-18.
[37] Antonucci, R. R .J., Ulvestad, J. S., Extended radio emission and the nature of blazars[J]. ApJ.,1985, 294:158.
[38] 白金明，谢光中。 BL Lac 天体处于高态与低态时的短时标光变的差异及机制研究[J]. 天体物理学报，1999,19（3）：240.
[39] Xie G.Z., Zhang X., Bai J.M. & Xie Z.H., Gamma-Rayand Near-Infraerd Emission form Gamma-Ray-loud Blazars[J].1998,ApJ,508:180.
[40] 樊军辉， G. E. Romero , ?瑞光。3C273 的光学光变周期[J] . 天文学报。 2001, 42（1）：9-15.
[41] Y. G. Zheng , X. Zhang , X. W. Bi , et al. Long-term Optical Spectra Variability of BL LacertaeObject OJ 287 [J] . MNRAS , 2008. 385 : 823-829.
[42] Horiuchi T. . A model of hydromagnetic turbulent viscosity in radiation-pressure-dominateddisks[J]. PASJ , 1990. 42, 661.
[43] 张雄，谢光中，白？明。 用 Jurkevich 方法分析计算 BLLac 天体的光变周期。 天体物学报。1998. 18 , 260.
[44] Foster G. Time Series Analysis by Projection.I.Statistical Properties of Fourier Analysis[J].AJ,1996, 111:541-55.
[45] Stiephane Mallat. A Wavelet Tour of Signal Processing[M].1999, USA:Academic Press 22-101.
[46] D'Arcangelo, F.D., Marscher, A.P., Jorstad, S.G., et al. Rapid Multiwaveband Polarization Variability in the Quasar PKS 0420-014: Optical Emission from the Compact Radio Jet[J], ApJ,2007, 659: L107-110.
[47] Blandford R.D. & Rees M.J., Some comments on radiation mechanisms in Lacertids[M].,Pittsburgh:Pittsburgh Univ. Press,1978,328:310.
[48] Pearson T.J., Zensus J.A., In Superluminal Radio Source[M].1987,Combridge:Combridge Univ.Press,P1.
[49] Perlman, E. S., Stocke, J. T., Wang, Q. D., et al. Soft X-Ray Observations of a Complete Sample of X-Ray-Selected BL lacertae Objects[J]. ApJ., 1996, 456:451.
[50] Antonucci, R. R .J., Ulvestad, J. S., Extended radio emission and the nature of blazars[J]. ApJ.,1985, 294:158.
[51] Keel .W. C., The jet of PKS 0521-36-an aging counterpart of M87?[J]. ApJ., 1986, 302:296.
[52] Stocke, J. T., liebert, J., Cshmids, G., et al. Optical and radio properties of X-ray selected BLLacertae objects[J]. ApJ., 1985, 298:619.
[53] Elvis M. et al., Most supenmassive black holes must be rapidly rotating[J].2002,ApJ, 565, L75.
[54] Ekers, R.D., Wall, J.V., Shaver, P. A., et al. A complete sample of radio galaxies. I-The radoi data[J]. MNRAS., 1989, 236:727.
[55] Sillanp?? A. et al.OJ 287-Binary pair of supermassive black holes [J].ApJ,1988,325: 628.
[56] Xie, G. Z., Zhang x., Bai, J. M., et al. Gamma-Ray and Nera-Infrared Emission from Gamma-ray-loud Blazars[J]. ApJ., 1998, 508:180.
[57] Wagner S.J.,Witzd A.,Intraday Variability In Quasars and BLLac objects[J],ARA&A,1995, 33,163.
[58] Dondi,L.,Ghisellini,G.,Gamma-ray-loud blazars and beaming[J].1995, MNRAS, 273:583.
[59] Storchi-Bergmann T.et al., The ionization cone, obscured nucleus, and gaseous outflow inNGC3281:A prototypical Seyfert II galaxy?[J].1992, ApJ, 396, 45.
[60] Storchi-Bergmann T.et al., The ionization cone, obscured nucleus, and gaseous outflow inNGC3281:A prototypical Seyfert II galaxy?[J].1992, ApJ, 396, 45.
[61] Hurt T.et al., Ultraviolet imaging polarimetry of narrow-line radio galaxies[J].1999,ApJ, 514,579.
[62] Pier E.A. and Krolik J.H., Infrared spectra of obscuring dust tori around active galactic nuclei.I.Calculational method and basic trends[J].1992,ApJ,401,99.
[63] Wilson A.S. & Tsvetanov Z.L, Ionization cones and radio ejects in active galaxies[J]. 1994, AJ,107,1227.
[64] Done C. et al., NGC4945: The brightest Seyfert II galaxy at 100keV[J].1996, ApJ, 463, L63.
[65] Biermann, P. L., Chirvasa, M., Falcke, H., et al. Single and binary Black Holes and their active environment[C], Proceedings of the 7eme Colloquium Cosmolo-gie, 'High Energy Astrophysics from and for Space' Paris, June 2002, Eds. N.Sanchez and H. de Vega, 11503（astro-ph/0211503）。
[66] Blandford R.D. & Rees M.J., Some comments on radiation mechanisms in Lacertids[M].Pittsburgh:Pittsburgh Univ. Press,1978, 328:310.
[67] Pearson T.J., Zensus J.A., In Superluminal Radio Source[M].1987,Combridge:Combridge Univ. Press,P1.
[68] D'Arcangelo, F.D., Marscher, A.P., Jorstad, S.G., et al. Rapid Multiwaveband Polarization Variability in the Quasar PKS 0420-014: Optical Emission from the Compact Radio Jet[J], ApJ,2007, 659: L107-110.
[69] Urry C.M. & Padovani P., Unified Schemes for Radio-Loud Active Galactic Nuclei[J].1995,PASP,107:803.
[70] Marscher, A.P., Jorstad, S.G., D'Arcangelo, F.D., et al. The inner jet of an active galactic nucleus as revealed by a radio-to-γ-ray outburst[J], Nature, 2008,452: 966-969.
[71] Hartman R.C., B?ttcher M., Aldering G.et al., Multiwavelength Spectra and Models for Blazar 3C 279[J].2001,ApJ,553:683.
[72] Xie G.Z., Lu J.F. & Wu J.X.et al., Determination of several parameters of BL Lacertae objects and relativistic beaming[J].1989,A&A,220:89.
[73] Sikora M., Begelman M.C., Rees M.J., Comptonization of diffuse ambient radiation by a
relativistic jet:The source of gamma rays from blazars?[J].1994,ApJ,421:153.
[74] Chiaberge,Marco.,Ghisellini,Gabriele.,Rapid variability in the synchrotron self-Compton model for blazars [J], 1999, MNRAS, 306: 551.
[75] Dermer C.D., Schlickeiser R., Model for the High-Energy Emission from Blazars[J]. 1993, ApJ,416:458.
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