Hostname: page-component-cd9895bd7-fscjk Total loading time: 0 Render date: 2024-12-25T19:46:52.620Z Has data issue: false hasContentIssue false
  • English
  • Français

How to detect supermassive binary black holes at parsec scales

Published online by Cambridge University Press:  07 March 2016

Xiang Liu
Xiang Liu*
Affiliation:
Xinjiang Astronomical Observatory of CAS, 150 Science 1-Street, Urumqi 830011, China email: liux@xao.ac.cn
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

It is difficult to find or identifying the binary black holes in parsec scales, since the dual AGN may be merged quickly. It is required to explore more possibilities to identifying binary black holes in parsec scales, we give some discussions, especially with the VLBI methods.

Keywords

black hole physics: binary – galaxies: jets – quasars: general – radio continuum
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Issue S312: Star Clusters and Black Holes in Galaxies across Cosmic Time , August 2014 , pp. 77 - 78
Copyright
Copyright © International Astronomical Union 2016 

References

Blecha, L., Loeb, A., & Narayan, R. 2013, MNRAS, 429, 2594CrossRefGoogle Scholar
Burke-Spolaor, S. 2011, MNRAS, 410, 2113CrossRefGoogle Scholar
Liu, X., Shen, Y., Bian, F. Y., et al. 2014, ApJ, 789, 140Google Scholar
Liu, X. 2014, J. Astrophys. Astr., Vol.35, No.3, 1Google Scholar
Liu, X., Mi, L.-G., Liu, B.-R., & Li, Q.-W. 2012, Ap&SS, 342, 465Google Scholar
Rodriguez, C., Taylor, G. B., Zavala, R. T., et al. 2006, ApJ, 646, 49Google Scholar
Smith, K. L., et al. 2010, ApJ, 716, 866Google Scholar
Wang, J.-M., et al. 2009, ApJ (Letters), 705, L76CrossRefGoogle Scholar