The prevalence of type III disc breaks in HI-rich and low-spin galaxies
文献类型：期刊论文
| 作者 | Wang, Jing2; Zheng, Zheng3; D'Souza, Richard4; Mo, Houjun5,6,7; Jozsa, Gyula8,9,10; Li, Cheng5,6; Kamphuis, Peter1,11; Catinella, Barbara12,13; Shao, Li2; Lagos, Claudia del P.12,14 |
| 刊名 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
 |
| 出版日期 | 2018-10-01 |
| 卷号 | 479期号:4页码:4292-4306 |
| 关键词 | galaxies: photometry galaxies: spiral galaxies: structure |
| ISSN号 | 0035-8711 |
| DOI | 10.1093/mnras/sty1687 |
| 英文摘要 | We investigate the origin of the type III (up-bending) discs based on a sample of 1808 galaxies from Sloan Digital Sky Survey and a sub-sample of 286 galaxies with HI data from ALFALFA. We examine how the type III fraction f(III), the fraction of disc galaxies which host up-bending disc breaks, depends on other galactic properties. We confirm that fIII strongly depends on the stellar concentration of galaxies. We find that HI-rich galaxies with low spins tend to have significantly more type III disc breaks than control galaxies, which are matched in concentration and stellar mass. This trend is independent of the existence of strong bars or environment of the galaxies. This result is broadly consistent with predictions from theoretical simulations, and indicates in situ star formation fuelled by gas accretion to be an important mechanism that builds the outer discs of type III galaxies. |
| WOS关键词 | DIGITAL SKY SURVEY ; ARECIBO SDSS SURVEY ; SPIRAL GALAXIES ; GALACTIC DISCS ; SURFACE PHOTOMETRY ; ELLIPTIC GALAXIES ; ANGULAR-MOMENTUM ; NEARBY GALAXIES ; STELLAR MASS ; DATA RELEASE |
| 资助项目 | Australian Research Council[DE150100618] ; National Key Basic Research Program of China[2015CB857004] ; National Natural Science Fundation of China (NSFC)[11173045] ; National Natural Science Fundation of China (NSFC)[11233005] ; National Natural Science Fundation of China (NSFC)[11325314] ; National Natural Science Fundation of China (NSFC)[11320101002] ; Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D)[CE170100013] ; NSF[AST-0607007] ; NSF[AST-1107390] ; Brinson Foundation ; Alfred P. Sloan Foundation ; National Science Foundation ; U.S. Department of Energy ; National Aeronautics and Space Administration ; Japanese Monbukagakusho ; Max Planck Society ; Higher Education Funding Council for England |
| WOS研究方向 | Astronomy & Astrophysics |
| 语种 | 英语 |
| WOS记录号 | WOS:000441383700002 |
| 出版者 | OXFORD UNIV PRESS |
| 资助机构 | Australian Research Council ; Australian Research Council ; National Key Basic Research Program of China ; National Key Basic Research Program of China ; National Natural Science Fundation of China (NSFC) ; National Natural Science Fundation of China (NSFC) ; Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D) ; Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D) ; NSF ; NSF ; Brinson Foundation ; Brinson Foundation ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; National Science Foundation ; National Science Foundation ; U.S. Department of Energy ; U.S. Department of Energy ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; Japanese Monbukagakusho ; Japanese Monbukagakusho ; Max Planck Society ; Max Planck Society ; Higher Education Funding Council for England ; Higher Education Funding Council for England ; Australian Research Council ; Australian Research Council ; National Key Basic Research Program of China ; National Key Basic Research Program of China ; National Natural Science Fundation of China (NSFC) ; National Natural Science Fundation of China (NSFC) ; Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D) ; Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D) ; NSF ; NSF ; Brinson Foundation ; Brinson Foundation ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; National Science Foundation ; National Science Foundation ; U.S. Department of Energy ; U.S. Department of Energy ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; Japanese Monbukagakusho ; Japanese Monbukagakusho ; Max Planck Society ; Max Planck Society ; Higher Education Funding Council for England ; Higher Education Funding Council for England ; Australian Research Council ; Australian Research Council ; National Key Basic Research Program of China ; National Key Basic Research Program of China ; National Natural Science Fundation of China (NSFC) ; National Natural Science Fundation of China (NSFC) ; Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D) ; Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D) ; NSF ; NSF ; Brinson Foundation ; Brinson Foundation ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; National Science Foundation ; National Science Foundation ; U.S. Department of Energy ; U.S. Department of Energy ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; Japanese Monbukagakusho ; Japanese Monbukagakusho ; Max Planck Society ; Max Planck Society ; Higher Education Funding Council for England ; Higher Education Funding Council for England ; Australian Research Council ; Australian Research Council ; National Key Basic Research Program of China ; National Key Basic Research Program of China ; National Natural Science Fundation of China (NSFC) ; National Natural Science Fundation of China (NSFC) ; Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D) ; Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D) ; NSF ; NSF ; Brinson Foundation ; Brinson Foundation ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; National Science Foundation ; National Science Foundation ; U.S. Department of Energy ; U.S. Department of Energy ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; Japanese Monbukagakusho ; Japanese Monbukagakusho ; Max Planck Society ; Max Planck Society ; Higher Education Funding Council for England ; Higher Education Funding Council for England |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/22500]  |
| 专题 | 中国科学院国家天文台 |
| 通讯作者 | Wang, Jing |
| 作者单位 | 1.Ruhr Univ Bochum, Astron Inst, Univ Str 150, D-44801 Bochum, Germany 2.Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China 3.Chinese Acad Sci, Natl Astron Observ, A20 Datun Rd, Beijing 100012, Peoples R China 4.Univ Michigan, Dept Astron, 1085 South Univ Ave, Ann Arbor, MI 48109 USA 5.Tsinghua Univ, Tsinghua Ctr Astrophys, Beijing 100084, Peoples R China 6.Tsinghua Univ, Dept Phys, Beijing 100084, Peoples R China 7.Univ Massachusetts, Dept Astron, Amherst, MA 01003 USA 8.Rhodes Univ, Dept Phys & Elect, Rhodes Ctr Radio Astron Tech & Technol, POB 94, ZA-6140 Grahamstown, South Africa 9.Argelander Inst Astron, Hugel 71, D-53121 Bonn, Germany 10.SKA South Africa Radio Astron Res Grp, 3rd Floor,Pk Rd, ZA-7405 Pinelands, South Africa |
| 推荐引用方式 GB/T 7714 | Wang, Jing,Zheng, Zheng,D'Souza, Richard,et al. The prevalence of type III disc breaks in HI-rich and low-spin galaxies[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2018,479(4):4292-4306. |
| APA | Wang, Jing.,Zheng, Zheng.,D'Souza, Richard.,Mo, Houjun.,Jozsa, Gyula.,...&Pan, Zhizheng.(2018).The prevalence of type III disc breaks in HI-rich and low-spin galaxies.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,479(4),4292-4306. |
| MLA | Wang, Jing,et al."The prevalence of type III disc breaks in HI-rich and low-spin galaxies".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 479.4(2018):4292-4306. |
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来源：国家天文台
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