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

页码：1032 / 1035

页数：4