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![]() | |
发表期刊 | ASTROPHYSICAL JOURNAL
![]() |
2012-04-01 | |
卷号 | 748期号:2 |
DOI | 10.1088/0004-637X/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 |
ISSN | 0004-637X |
URL | 查看原文 |
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 |
引用统计 | |
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 |
推荐引用方式 GB/T 7714 | 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). |
条目包含的文件 | ||||||
文件名称/大小 | 文献类型 | 版本类型 | 开放类型 | 使用许可 | ||
THE CENTRAL ENGINES (473KB) | 期刊论文 | 作者接受稿 | 开放获取 | CC BY-NC-SA | 浏览 请求全文 |
除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。
修改评论