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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
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)
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页码:1032 / 1035
页数:4
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