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Black hole mass and radiation pressure of Seyfert 1 galaxies

Xiong Ding-Rong Zhang Xiong Zheng Yong-Gang Huang Bang-Rong Mao Li-Sheng Liu Wen-Guang Cha Yong-Juan

Black hole mass and radiation pressure of Seyfert 1 galaxies

Xiong Ding-Rong, Zhang Xiong, Zheng Yong-Gang, Huang Bang-Rong, Mao Li-Sheng, Liu Wen-Guang, Cha Yong-Juan
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  • We collect 214 Seyfert 1 galaxies(147 narrow line Seyfert 1 and 67 broad line Seyfert 1) and research black hole mass bulge velocity dispersion Eddington radio luminosity at 5100 Å and redshift. Our conclusions are follows: (1) when computing black hole mass, we should consider the effect of radiation pressure, especially for the narrow line Seyfert 1 galaxies; (2) when the effect of radiation pressure is considered, narrow line Seyfert 1 galaxies meet MBH-σ relation of normal galaxies and are in su-Eddington accretion; (3) in a large samples, the evolution of Seyfert 1 galaxies is from narrow line Seyfert 1 galaxies to broad line Seyfert 1 galaxies, which is consistent with other results obtained in different ways.
    • Funds: Project supported by the National Natural Science Foundation of China (Grant No. 11163007), the Gravitational Theory Innovation Team of Yunnan Provincial of China and High Energy Astrophysics of University Innovation Team of Yunnan Provincial of China.
    [1]

    Croton D J, Springel V, White S D M, DeLucia G, Frenk C S, Gao L, Jenkins A, Kauffmann G, Navarro J F, Yoshida N 2006 Mon. Not. R. Astron. Soc. 365 11

    [2]

    Ferrarese L, Merritt D 2000 Astrophys. J. 539 L9

    [3]

    Marconi A, Hunt L K 2003 Astrophys. J. L21

    [4]

    Graham A W, Driver S P 2007 Astrophys. J. 655 77

    [5]

    Granato G L, DeZotti G, Silva L, Bresssan A, Danese L 2004 Astrophys. J. 600 580

    [6]

    Kaspi S, Smith P S, Netzer H, Maoz D, Jannuzi B T, Giveon U 2000 Astrophys. J. 533 631

    [7]

    Onken C A, Ferrarese L, Merritt D, Peterson B M, Pogge R W, Vestergaard M, Wandel A 2004 Astrophys. J. 615 645

    [8]

    Vestergaard M, Peterson B M 2006 Astrophys. J. 641 689

    [9]

    Woo J H, Treu T, Barth A J, Wright S A, Walsh J L, Bentz M C, Martini P, Bennert A N, Canalizo G, Filippenko A V, Gates E, Greene J, Malkan M A, Stern D, Minezaki T 2010 Astrophys. J. 716 269

    [10]

    Marconi A, Axon D J, Maiolino R, Nagao T, Pastorini G, Pietrini P, Robinson A, Torricelli G 2008 Astrophys. J. 678 693

    [11]

    Marconi A, Axon D J, Maiolino R, Nagao T, Pastorini G, Pietrini P, Robinson A, Torricelli G 2009 Astrophys. J. 698 L103

    [12]

    Zhu L, Zhang S N, Tang S 2009 Astrophys. J. 700 1173

    [13]

    Tremaine S, Gebhardt K, Bender R, Bower G, Dressler A, Faber S M, Filippenko A V, Green R, Grillmair G, Ho L C, Kormendy J, Lauer T R, Magorrian J, Pinkney J, Richstone D 2002 Astrophys. J. 574 740

    [14]

    Greene J E, Ho L C 2006 Astrophys. J. 641 L21

    [15]

    Bian W, Zhao Y 2004 Mon. Not. R. Astron. Soc. 352 823

    [16]

    Komossa S, Xu D 2007 Astrophys. J. 667 L33

    [17]

    Wang J M, Zhang E P 2007 Astrophys. J. 660 1072

    [18]

    Xie G Z, Zhou S B, Liang E W 2004 Astron. J. 127 53

    [19]

    Bao Y Y, Zhang X, Chen L E, Zhang H J, Peng Z Y, Zheng Y G 2008 Acta Astron. Sin. 49 123 (in Chinese) [鲍玉英, 张雄, 陈洛恩, 张皓晶, 彭朝阳, 郑永刚 2008 天文学报 49 123]

    [20]

    Pei Y C 1995 Astrophys. J. 438 623

  • [1]

    Croton D J, Springel V, White S D M, DeLucia G, Frenk C S, Gao L, Jenkins A, Kauffmann G, Navarro J F, Yoshida N 2006 Mon. Not. R. Astron. Soc. 365 11

    [2]

    Ferrarese L, Merritt D 2000 Astrophys. J. 539 L9

    [3]

    Marconi A, Hunt L K 2003 Astrophys. J. L21

    [4]

    Graham A W, Driver S P 2007 Astrophys. J. 655 77

    [5]

    Granato G L, DeZotti G, Silva L, Bresssan A, Danese L 2004 Astrophys. J. 600 580

    [6]

    Kaspi S, Smith P S, Netzer H, Maoz D, Jannuzi B T, Giveon U 2000 Astrophys. J. 533 631

    [7]

    Onken C A, Ferrarese L, Merritt D, Peterson B M, Pogge R W, Vestergaard M, Wandel A 2004 Astrophys. J. 615 645

    [8]

    Vestergaard M, Peterson B M 2006 Astrophys. J. 641 689

    [9]

    Woo J H, Treu T, Barth A J, Wright S A, Walsh J L, Bentz M C, Martini P, Bennert A N, Canalizo G, Filippenko A V, Gates E, Greene J, Malkan M A, Stern D, Minezaki T 2010 Astrophys. J. 716 269

    [10]

    Marconi A, Axon D J, Maiolino R, Nagao T, Pastorini G, Pietrini P, Robinson A, Torricelli G 2008 Astrophys. J. 678 693

    [11]

    Marconi A, Axon D J, Maiolino R, Nagao T, Pastorini G, Pietrini P, Robinson A, Torricelli G 2009 Astrophys. J. 698 L103

    [12]

    Zhu L, Zhang S N, Tang S 2009 Astrophys. J. 700 1173

    [13]

    Tremaine S, Gebhardt K, Bender R, Bower G, Dressler A, Faber S M, Filippenko A V, Green R, Grillmair G, Ho L C, Kormendy J, Lauer T R, Magorrian J, Pinkney J, Richstone D 2002 Astrophys. J. 574 740

    [14]

    Greene J E, Ho L C 2006 Astrophys. J. 641 L21

    [15]

    Bian W, Zhao Y 2004 Mon. Not. R. Astron. Soc. 352 823

    [16]

    Komossa S, Xu D 2007 Astrophys. J. 667 L33

    [17]

    Wang J M, Zhang E P 2007 Astrophys. J. 660 1072

    [18]

    Xie G Z, Zhou S B, Liang E W 2004 Astron. J. 127 53

    [19]

    Bao Y Y, Zhang X, Chen L E, Zhang H J, Peng Z Y, Zheng Y G 2008 Acta Astron. Sin. 49 123 (in Chinese) [鲍玉英, 张雄, 陈洛恩, 张皓晶, 彭朝阳, 郑永刚 2008 天文学报 49 123]

    [20]

    Pei Y C 1995 Astrophys. J. 438 623

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  • Received Date:  31 March 2012
  • Accepted Date:  13 June 2012
  • Published Online:  20 November 2012

Black hole mass and radiation pressure of Seyfert 1 galaxies

  • 1. College of Physics and Electronics, Yunnan Normal University, Kunming 650092, China
Fund Project:  Project supported by the National Natural Science Foundation of China (Grant No. 11163007), the Gravitational Theory Innovation Team of Yunnan Provincial of China and High Energy Astrophysics of University Innovation Team of Yunnan Provincial of China.

Abstract: We collect 214 Seyfert 1 galaxies(147 narrow line Seyfert 1 and 67 broad line Seyfert 1) and research black hole mass bulge velocity dispersion Eddington radio luminosity at 5100 Å and redshift. Our conclusions are follows: (1) when computing black hole mass, we should consider the effect of radiation pressure, especially for the narrow line Seyfert 1 galaxies; (2) when the effect of radiation pressure is considered, narrow line Seyfert 1 galaxies meet MBH-σ relation of normal galaxies and are in su-Eddington accretion; (3) in a large samples, the evolution of Seyfert 1 galaxies is from narrow line Seyfert 1 galaxies to broad line Seyfert 1 galaxies, which is consistent with other results obtained in different ways.

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