ACTIVE GALACTIC NUCLEUS PAIRS FROM THE SLOAN DIGITAL SKY SURVEY. I. THE FREQUENCY ON similar to 5-100 kpc SCALES
文献类型:期刊论文
| 作者 | Liu, Xin1,2; Shen, Yue1; Strauss, Michael A.2; Hao, Lei3
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| 刊名 | ASTROPHYSICAL JOURNAL
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| 出版日期 | 2011-08-20 |
| 卷号 | 737期号:2页码:1 |
| 关键词 | black hole physics galaxies: active galaxies: interactions galaxies: nuclei quasars: general |
| 英文摘要 | Galaxy-galaxy mergers and close interactions have long been regarded as a viable mechanism for channeling gas toward the central supermassive black holes (SMBHs) of galaxies which are triggered as active galactic nuclei (AGNs). AGN pairs, in which the central SMBHs of a galaxy merger are both active, are expected to be common from such events. We conduct a systematic study of 1286 AGN pairs at (z) over bar similar to 0.1 with line-of-sight velocity offsets Delta v < 600 km s(-1) and projected separations r(p) < 100 h(70)(-1) kpc, selected from the Seventh Data Release of the Sloan Digital Sky Survey (SDSS). This AGN pair sample was drawn from 138,070 AGNs optically identified based on diagnostic emission line ratios and/or line widths. The fraction of AGN pairs with 5 h(70)(-1) kpc less than or similar to r(p) < 100 h(70)(-1) kpc among all spectroscopically selected AGNs at 0.02 < z < 0.16 is 3.6% after correcting for SDSS spectroscopic incompleteness; similar to 30% of these pairs show morphological tidal features in their SDSS images, and the fraction becomes greater than or similar to 80% for pairs with the brightest nuclei. Our sample increases the number of known AGN pairs on these scales by more than an order of magnitude. We study their AGN and host-galaxy star formation properties in a companion paper. |
| WOS标题词 | Science & Technology ; Physical Sciences |
| 类目[WOS] | Astronomy & Astrophysics |
| 研究领域[WOS] | Astronomy & Astrophysics |
| 关键词[WOS] | SUPERMASSIVE BLACK-HOLES ; SPECTROSCOPIC TARGET SELECTION ; STAR-FORMING GALAXIES ; NARROW-LINE REGION ; 7TH DATA RELEASE ; SIMILAR-TO 3-4 ; HOST GALAXIES ; BINARY QUASARS ; METALLICITY RELATION ; FORMATION HISTORIES |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000294013600055 |
| 源URL | [http://119.78.226.72/handle/331011/26401] ![]() |
| 专题 | 上海天文台_星系宇宙学重点实验室 |
| 作者单位 | 1.Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA 2.Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA 3.Chinese Acad Sci, Shanghai Astron Observ, Shanghai 200030, Peoples R China |
| 推荐引用方式 GB/T 7714 | Liu, Xin,Shen, Yue,Strauss, Michael A.,et al. ACTIVE GALACTIC NUCLEUS PAIRS FROM THE SLOAN DIGITAL SKY SURVEY. I. THE FREQUENCY ON similar to 5-100 kpc SCALES[J]. ASTROPHYSICAL JOURNAL,2011,737(2):1. |
| APA | Liu, Xin,Shen, Yue,Strauss, Michael A.,&Hao, Lei.(2011).ACTIVE GALACTIC NUCLEUS PAIRS FROM THE SLOAN DIGITAL SKY SURVEY. I. THE FREQUENCY ON similar to 5-100 kpc SCALES.ASTROPHYSICAL JOURNAL,737(2),1. |
| MLA | Liu, Xin,et al."ACTIVE GALACTIC NUCLEUS PAIRS FROM THE SLOAN DIGITAL SKY SURVEY. I. THE FREQUENCY ON similar to 5-100 kpc SCALES".ASTROPHYSICAL JOURNAL 737.2(2011):1. |
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来源:上海天文台
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