A massive binary black-hole system in OJ 287 and a test of general relativity

被引:315
|
作者
Valtonen, M. J. [1 ,2 ]
Lehto, H. J. [1 ,2 ]
Nilsson, K. [2 ]
Heidt, J. [3 ]
Takalo, L. O. [1 ,2 ]
Sillanpaa, A. [1 ,2 ]
Villforth, C. [1 ,2 ]
Kidger, M. [4 ,5 ]
Poyner, G. [6 ]
Pursimo, T. [7 ]
Zola, S. [8 ]
Wu, J. -H. [10 ]
Zhou, X. [10 ]
Sadakane, K. [11 ]
Drozdz, M.
Koziel, D. [8 ]
Marchev, D. [12 ]
Ogloza, W.
Porowski, C. [8 ]
Siwak, M. [8 ]
Stachowski, G. [9 ]
Winiarski, M. [8 ]
Hentunen, V. -P.
Nissinen, M. [13 ]
Liakos, A. [14 ]
Dogru, S. [15 ]
机构
[1] Univ Turku, Dept Phys, FI-21500 Piikkio, Finland
[2] Univ Turku, Tuorla Observ, FI-21500 Piikkio, Finland
[3] Landessternwarte Heidelberg, D-69117 Heidelberg, Germany
[4] European Space Agcy, European Space Astron Ctr, Herschel Sci Ctr, Villafrance Castillo Satellite Tracking Stn, Madrid 28691, Spain
[5] INSA, Madrid 28008, Spain
[6] British Astron Assoc Variable Star Sect, Birmingham B44 0QE, W Midlands, England
[7] Nord Opt Telescope, E-38700 S C La Palma, Spain
[8] Jagiellonian Univ, Astron Observ, PL-30224 Krakow, Poland
[9] Pedagog Univ, Mt Suhora Observ, PL-30084 Krakow, Poland
[10] Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
[11] Osaka Kyoiku Univ, Inst Astron, Kashiwara, Osaka 5828582, Japan
[12] Shoumen Univ, Dept Phys, Shumen, Bulgaria
[13] Warkauden Kassiopeia Ry, Kangaslampi 79480, Finland
[14] Univ Athens, Fac Phys, Dept Astrophys Astron & Mech, GR-15784 Athens, Greece
[15] Canakkale Onsekiz Mart Univ, Fac Phys, TR-17020 Canakkale, Turkey
关键词
D O I
10.1038/nature06896
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
Tests of Einstein's general theory of relativity have mostly been carried out in weak gravitational fields where the space- time curvature effects are first- order deviations from Newton's theory(1-6). Binary pulsars(4) provide a means of probing the strong gravitational field around a neutron star, but strong- field effects may be best tested in systems containing black holes(7,8). Here we report such a test in a close binary system of two candidate black holes in the quasar OJ 287. This quasar shows quasi- periodic optical outbursts at 12- year intervals, with two outburst peaks per interval(9,10). The latest outburst occurred in September 2007, within a day of the time predicted by the binary black- hole model and general relativity(11). The observations confirm the binary nature of the system and also provide evidence for the loss of orbital energy in agreement ( within 10 per cent) with the emission of gravitational waves from the system(12). In the absence of gravitational wave emission the outburst would have happened 20 days later(13).
引用
收藏
页码:851 / 853
页数:3
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