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THE CENTRAL ENGINES OF TWO UNUSUAL RADIO-INTERMEDIATE/QUIET ACTIVE GALACTIC NUCLEI: III Zw 2 AND PG 1407+265
Chen, L1; Cao, XW1; Bai JM(白金明)2,3; Chen, L (reprint author), Chinese Acad Sci, Key Lab Res Galaxies & Cosmol, Shanghai Astron Observ, 80 Nandan Rd, Shanghai 200030, Peoples R China.
发表期刊ASTROPHYSICAL JOURNAL
2012-04-01
卷号748期号:2
DOI10.1088/0004-637X/748/2/119
产权排序第2完成单位
收录类别SCI
关键词Galaxies: Active Galaxies: Jets Quasars: Individual (Iii Zw 2 And Pg 1407+265) Radiation Mechanisms: Non-thermal Radiation Mechanisms: Thermal
摘要We use the accretion disk/corona + jet model to fit the multi-band spectral energy distributions (SEDs) of two unusual radio-intermediate/quiet quasars. It is found that the optical/UV emission of III Zw 2 is probably dominated by the emission from the accretion disk. The X-ray emission should be dominated by the radiation from the jet, while the contribution of the disk corona is negligible. The optical/UV component in the SED of PG 1407+265 can be well modeled as the emission from the accretion disk, while the IR component is attributed to the thermal radiation from the dust torus with an opening angle of similar to 50 degrees. If the X-ray continuum emission is dominated by the synchrotron emission of the jet, the source should be a "high peak frequency blazar," which obviously deviates from the normal blazar sequence. The observed SED can also be fitted quite well by the accretion disk/corona model with the viscosity parameter alpha = 0.5. The spectrum of the accretion disk/corona in PG 1407+265 satisfies the weak-line quasar criterion suggested in Laor & Davis.
项目资助者NSFC [10821302, 10833002, 11173043, 11133006, 10973034, 10903025, 11078008, 11103060] ; National Basic Research Program of China [2009CB824800] ; Science and Technology Commission of Shanghai Municipality [10XD1405000] ; CAS/SAFEA [KJCX2-YW-T23]
语种英语
学科领域Astronomy & Astrophysics
文章类型Article
ISSN0004-637X
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WOS记录号WOS:000302135200047
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]X-RAY-SPECTRA ; ACCRETION DISK MODELS ; BRIGHT QUASAR SURVEY ; PALOMAR-GREEN QUASARS ; LARGE-AREA TELESCOPE ; QUIET QUASARS ; ENERGY-DISTRIBUTIONS ; RELATIVISTIC JET ; SEYFERT-GALAXY ; BLACK-HOLES
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被引频次:19[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/5423
专题南方基地
中国科学院天体结构与演化重点实验室
通讯作者Chen, L (reprint author), Chinese Acad Sci, Key Lab Res Galaxies & Cosmol, Shanghai Astron Observ, 80 Nandan Rd, Shanghai 200030, Peoples R China.
作者单位1.Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai 200030, China
2.National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, Kunming 650011, China
3.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650011, China
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Chen, L,Cao, XW,Bai JM,et al. THE CENTRAL ENGINES OF TWO UNUSUAL RADIO-INTERMEDIATE/QUIET ACTIVE GALACTIC NUCLEI: III Zw 2 AND PG 1407+265[J]. ASTROPHYSICAL JOURNAL,2012,748(2).
APA Chen, L,Cao, XW,Bai JM,&Chen, L .(2012).THE CENTRAL ENGINES OF TWO UNUSUAL RADIO-INTERMEDIATE/QUIET ACTIVE GALACTIC NUCLEI: III Zw 2 AND PG 1407+265.ASTROPHYSICAL JOURNAL,748(2).
MLA Chen, L,et al."THE CENTRAL ENGINES OF TWO UNUSUAL RADIO-INTERMEDIATE/QUIET ACTIVE GALACTIC NUCLEI: III Zw 2 AND PG 1407+265".ASTROPHYSICAL JOURNAL 748.2(2012).
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