期刊文献+

Feedback of Active Galactic Nuclei in Seyfert 2 Galaxies

Feedback of Active Galactic Nuclei in Seyfert 2 Galaxies
下载PDF
导出
摘要 It is well accepted that feedback from active galactic nuclei (AGNs) plays an important role in the coevolution of the supermassive black hole (SMBH) and its host galaxy, but the concrete mechanism of feedback remains unclear. A considerable body of evidence suggests that AGN feedback suppresses star formation in the host galaxy. We assemble a sample of Seyfert 2 galaxies with recent observational data of compact nuclear starbursts and estimate the gas surface density as a function of column density to illuminate the relation between feedback and AGN properties. Although there are some uncertainties, our data still imply the deviation from the star formation law (Kennicutt-Schmidt law). Further, they indicate that: (1) Feedback correlates with the Eddington ratio, rather than with the mass of SMBH, as a result of decreasing star formation efficiency. (2) The SMBH and the torus are probably undergoing coevolution. Conclusions presented here can be refined through future high resolution CO or HCN observations. It is well accepted that feedback from active galactic nuclei (AGNs) plays an important role in the coevolution of the supermassive black hole (SMBH) and its host galaxy, but the concrete mechanism of feedback remains unclear. A considerable body of evidence suggests that AGN feedback suppresses star formation in the host galaxy. We assemble a sample of Seyfert 2 galaxies with recent observational data of compact nuclear starbursts and estimate the gas surface density as a function of column density to illuminate the relation between feedback and AGN properties. Although there are some uncertainties, our data still imply the deviation from the star formation law (Kennicutt-Schmidt law). Further, they indicate that: (1) Feedback correlates with the Eddington ratio, rather than with the mass of SMBH, as a result of decreasing star formation efficiency. (2) The SMBH and the torus are probably undergoing coevolution. Conclusions presented here can be refined through future high resolution CO or HCN observations.
出处 《Chinese Journal of Astronomy and Astrophysics》 CSCD 2008年第5期537-546,共10页 中国天文和天体物理学报(英文版)
基金 the National Natural Science Foundation of China
关键词 galaxies active - galaxies Seyfert- feedback galaxies active - galaxies Seyfert- feedback
  • 相关文献

参考文献69

  • 1Antonucci R. R. J., 1993, ARA&A, 31,473
  • 2Bassani L. et al., 1999, ApJS, 121,473
  • 3Bian W.-H., Zhao Y.-H., 2003, Chin. J. Astron. Astrophys. (ChJAA), 3, 119
  • 4Bian W.-H., Cui Q.-L. Chao L.-H., 2006, Chin. J. Astron. Astrophys. (ChJAA), 6, 281
  • 5Cid Fernandes R. et al., 2001, ApJ, 558, 81
  • 6Croton D. J. et al., 2006, MNRAS, 365, 11
  • 7Dahari O., De Robertis M. M., 1988, ApJS, 67, 249
  • 8Davies R. I., Mueller S. F., Genzel R. et al., 2007, ApJ, 671, 1388
  • 9de Grijp M. H. K., Keel W. C., Miley G. K. et al., 1992, A&AS, 96, 389
  • 10De Robertis M. M., Hayhoe K., Yee H. K. C., 1998, 115, 163

相关作者

内容加载中请稍等...

相关机构

内容加载中请稍等...

相关主题

内容加载中请稍等...

浏览历史

内容加载中请稍等...
;
使用帮助 返回顶部