A Ringed Dwarf LINER 1 Galaxy Hosting an Intermediate-mass Black Hole with Large-scale Rotation-like Emission
文献类型：期刊论文
| 作者 | Liu,Wen-Juan1,10,11; Qian,Lei1,2; Dong,Xiao-Bo1,10,11; Jiang,Ning3; Lira,Paulina4; Cai,Zheng5; Wang,Feige6; Yang,Jinyi6; Xiao,Ting7; Kim,Minjin8,9 |
| 刊名 | The Astrophysical Journal
 |
| 出版日期 | 2017-03-08 |
| 卷号 | 837期号:2 |
| 关键词 | galaxies: active galaxies: dwarf galaxies: individual (SDSS J083803.68+540642.0) galaxies: nuclei galaxies: Seyfert |
| ISSN号 | 0004-637X |
| DOI | 10.3847/1538-4357/aa5eb6 |
| 英文摘要 | Abstract We report the discovery of a 20 kpc sized emission in SDSS J083803.68+540642.0, a ringed dwarf galaxy ( mag) hosting an accreting intermediate-mass black hole at z?=?0.02957. Analysis of the Hubble Space Telescope images indicates that it is an early-type galaxy with a featureless low-surface brightness disk ( mag?arcsec?2 in the V band) and a prominent, relatively red bulge (V ? I?=?2.03, or 0.″48) that accounts for ≈81% of the total light in the I band. A circumgalactic ring of a diameter 16 kpc is also detected, with a disperse shape on its south side. The optical emission lines reveal the nucleus to be a broad-line LINER. Our MMT longslit observation indicates that the kinematics of the extended emission is consistent with a rotational gaseous disk, with a mean blueshifted velocity of 162 and mean redshifted velocity of 86 . According to our photoionization calculations, the large-scale emission is unlikely to be powered by the central nucleus or by hot evolved (post-AGB) stars interspersed in the old stellar populations, but by in situ star formation; this is vindicated by the line-ratio diagnostic of the extended emission. We propose that both the ring and large-scale -emitting gas are created by the tidal accretion in a collision—and then merger—with a gas-rich galaxy of a comparable mass. |
| 语种 | 英语 |
| WOS记录号 | IOP:0004-637X-837-2-AA5EB6 |
| 出版者 | The American Astronomical Society |
| 源URL | [http://119.78.226.72/handle/331011/32135]  |
| 专题 | 中国科学院上海天文台 |
| 作者单位 | 1.Center for Astronomical Mega-Science, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing, 100012, P. R. China 2.National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100012, China 3.Department of Astronomy, University of Science and Technology of China, Hefei, Anhui 230026, China 4.Departamento de Astronomía, Universidad de Chile, Casilla 36-D, Santiago, Chile 5.UCO/Lick Observatory, University of California, 1156 High Street, Santa Cruz, CA 95064, USA 6.Department of Astronomy, School of Physics, Peking University, Beijing 100871, China 7.Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai 200030, China 8.Korea Astronomy and Space Science Institute, Daejeon 305-348, Korea 9.University of Science and Technology, Daejeon 305-350, Korea 10.Yunnan Observatories, Chinese Academy of Sciences, Kunming, Yunnan 650011, China; wjliu@ynao.ac.cn; xbdong@ynao.ac.cn |
| 推荐引用方式 GB/T 7714 | Liu,Wen-Juan,Qian,Lei,Dong,Xiao-Bo,et al. A Ringed Dwarf LINER 1 Galaxy Hosting an Intermediate-mass Black Hole with Large-scale Rotation-like Emission[J]. The Astrophysical Journal,2017,837(2). |
| APA | Liu,Wen-Juan.,Qian,Lei.,Dong,Xiao-Bo.,Jiang,Ning.,Lira,Paulina.,...&Kim,Minjin.(2017).A Ringed Dwarf LINER 1 Galaxy Hosting an Intermediate-mass Black Hole with Large-scale Rotation-like Emission.The Astrophysical Journal,837(2). |
| MLA | Liu,Wen-Juan,et al."A Ringed Dwarf LINER 1 Galaxy Hosting an Intermediate-mass Black Hole with Large-scale Rotation-like Emission".The Astrophysical Journal 837.2(2017). |
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来源：上海天文台
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