BROAD-LINE RADIO GALAXIES OBSERVED WITH FERMI-LAT: THE ORIGIN OF THE GeV γ-RAY EMISSION

被引:64
作者
Kataoka, J. [1 ]
Stawarz, L. [2 ,3 ]
Takahashi, Y. [1 ]
Cheung, C. C. [4 ]
Hayashida, M. [5 ,7 ]
Grandi, P. [6 ]
Burnett, T. H. [8 ]
Celotti, A. [9 ]
Fegan, S. J. [10 ]
Fortin, P. [10 ]
Maeda, K. [1 ]
Nakamori, T. [1 ]
Taylor, G. B. [11 ]
Tosti, G. [12 ,13 ]
Digel, S. W. [5 ,7 ]
McConville, W. [14 ,15 ,16 ]
Finke, J. [17 ]
D'Ammando, F. [18 ,19 ]
机构
[1] Waseda Univ, Res Inst Sci & Engn, Tokyo 1698555, Japan
[2] JAXA, Inst Space & Astronaut Sci, Kanagawa 2525210, Japan
[3] Jagiellonian Univ, Astron Observ, PL-30244 Krakow, Poland
[4] Natl Acad Sci, Washington, DC 20001 USA
[5] Stanford Univ, WW Hansen Expt Phys Lab, Kavli Inst Particle Astrophys & Cosmol, Dept Phys, Stanford, CA 94305 USA
[6] INAF IASF Bologna, I-40129 Bologna, Italy
[7] Stanford Univ, SLAC Natl Accelerator Lab, Stanford, CA 94305 USA
[8] Univ Washington, Dept Phys, Seattle, WA 98195 USA
[9] SISSA, I-34014 Trieste, Italy
[10] Ecole Polytech, CNRS, Lab Leprince Ringuet, IN2P3, F-91128 Palaiseau, France
[11] Univ New Mexico, Dept Phys & Astron, Albuquerque, NM 87131 USA
[12] Ist Nazl Fis Nucl, Sez Perugia, I-06123 Perugia, Italy
[13] Univ Perugia, Dipartimento Fis, I-06123 Perugia, Italy
[14] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[15] Univ Maryland, Dept Phys, College Pk, MD 20742 USA
[16] Univ Maryland, Dept Astron, College Pk, MD 20742 USA
[17] USN, Res Lab, Div Space Sci, Washington, DC 20375 USA
[18] IASF Palermo, I-90146 Palermo, Italy
[19] INAF Ist Astrofis Spaziale & Fis Cosm, I-00133 Rome, Italy
基金
美国国家航空航天局; 美国国家科学基金会; 瑞典研究理事会;
关键词
galaxies: active; galaxies:; individual; (3C; 120; 3C; 111); galaxies: jets; gamma rays: galaxies; radiation mechanisms: non-thermal; X-rays: galaxies; ACTIVE GALACTIC NUCLEI; LARGE-AREA TELESCOPE; ADVECTION-DOMINATED ACCRETION; BLACK-HOLE MASS; XMM-NEWTON OBSERVATION; BRIGHT QUASAR SURVEY; ALL-SKY SURVEY; X-RAY; VLBI OBSERVATIONS; COMPLETE SAMPLE;
D O I
10.1088/0004-637X/740/1/29
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report on a detailed investigation of the gamma-ray emission from 18 broad-line radio galaxies (BLRGs) based on two years of Fermi Large Area Telescope data. We confirm the previously reported detections of 3C 120 and 3C 111 in the GeV photon energy range; a detailed look at the temporal characteristics of the observed gamma-ray emission reveals in addition possible flux variability in both sources. No statistically significant gamma-ray detection of the other BLRGs was found, however, in the considered data set. Though the sample size studied is small, what appears to differentiate 3C 111 and 3C 120 from the BLRGs not yet detected in gamma-rays is the particularly strong nuclear radio flux. This finding, together with the indications of the gamma-ray flux variability and a number of other arguments presented, indicates that the GeV emission of BLRGs is most likely dominated by the beamed radiation of relativistic jets observed at intermediate viewing angles. In this paper we also analyzed a comparison sample of high-accretion-rate Seyfert 1 galaxies, which can be considered radio-quiet counterparts of BLRGs, and found that none were detected in gamma-rays. A simple phenomenological hybrid model applied for the broadband emission of the discussed radio-loud and radio-quiet type 1 active galaxies suggests that the relative contribution of the nuclear jets to the accreting matter is >= 1% on average for BLRGs, whereas it is <= 0.1% for Seyfert 1 galaxies.
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页数:16
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