Supermassive black hole mergers as dual sources for electromagnetic flares in the jet emission and gravitational waves

被引：4
|
作者：
Tapai, M. [1 ]
Gergely, L. A. [1 ,2 ]
Keresztes, Z. [1 ]
Wiita, P. J. [3 ]
Gopal-Krishna [4 ]
Biermann, P. L. [5 ,6 ,7 ,8 ,9 ]
机构：
[1] Univ Szeged, Dept Theoret & Expt Phys, H-6720 Szeged, Hungary
[2] Tokyo Univ Sci, Dept Phys, Shinjuku Ku, Tokyo 1628601, Japan
[3] Coll New Jersey, Dept Phys, Ewing, NJ 08628 USA
[4] Interuniv Ctr Astron & Astrophys IUCAA, Pune 411007, Maharashtra, India
[5] Max Planck Inst Radioastron, D-53121 Bonn, Germany
[6] Univ Bonn, Dept Phys & Astron, Bonn, Germany
[7] Univ Alabama, Dept Phys & Astron, Tuscaloosa, AL 35487 USA
[8] Univ Alabama, Dept Phys, Huntsville, AL 35899 USA
[9] Karlsruher Inst Technol, Inst Nucl Phys, D-76021 Karlsruhe, Germany
来源：
ASTRONOMISCHE NACHRICHTEN | 2013年 / 334卷 / 09期
基金：
日本学术振兴会;
关键词：
black hole physics; galaxies: binary; galaxies: jets; gravitational waves; ACTIVE GALACTIC NUCLEI; SPECTRUM RADIO-SOURCES; COMPLETE SAMPLE; EFFICIENT MERGER; STANDARD SIRENS; BINARY MERGERS; GAS DISCS; S5; SURVEY; COUNTERPARTS; GALAXIES;
D O I：
10.1002/asna.201211988
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We present a new type of observation relating the gravitational wave emission of supermassive black hole mergers to their electromagnetic counterparts. This dual emission involves variability of a relativistic jet arising from the spin-orbit precession of the supermassive black hole binary at its base. ((c) 2013 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim)
引用
收藏
页码：1032 / 1035
页数：4
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