Far-infrared Herschel SPIRE spectroscopy of lensed starbursts reveals physical conditions of ionized gas
文献类型:期刊论文
作者 | Zhang, Zhi-Yu1,2; Ivison, R. J.1,2; George, R. D.1; Zhao, Yinghe3,4,5; Dunne, L.1,6; Herrera-Camus, R.7; Lewis, A. J. R.1; Liu, Daizhong8,9; Naylor, D.10; Oteo, Ivan1,2 |
刊名 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY |
出版日期 | 2018-11-01 |
卷号 | 481期号:1页码:59-97 |
ISSN号 | 0035-8711 |
关键词 | galaxies: active galaxies: high-redshift galaxies: starburst infrared: galaxies submillimetre: galaxies |
DOI | 10.1093/mnras/sty2082 |
英文摘要 | The most intensively star-forming galaxies are extremely luminous at far-infrared ( FIR) wavelengths, highly obscured at optical and ultraviolet wavelengths, and lie at z >= 1-3. We present a programme of FIR spectroscopic observations with the SPIRE FTS, as well as photometric observations with PACS, both on board Herschel, towards a sample of 45 gravitationally lensed, dusty starbursts across z similar to 1-3.6. In total, we detected 27 individual lines down to 3 sigma, including nine [C II] 158 mu m lines with confirmed spectroscopic redshifts, five possible [C II] lines consistent with their FIR photometric redshifts, and in some individual sources a few [OIII] 88 mu m, [O III] 52 mu m, [O I] 145 mu m, [O I] 63 mu m, [N II] 122 mu m and OH 119 mu m ( in absorption) lines. To derive the typical physical properties of the gas in the sample, we stack all spectra weighted by their intrinsic luminosity and by their 500 mu m flux densities, with the spectra scaled to a common redshift. In the stacked spectra, we detect emission lines of [CII] 158 mu m, [N II] 122 mu m, [O III] 88 mu m, [O III] 52 mu m, [O I] 63 mu m and the absorption doublet of OH at 119 mu m, at high fidelity. We find that the average electron densities traced by the [NII] and [O III] lines are higher than the average values in local star-forming galaxies and ULIRGs, using the same tracers. From the [NII]/[C II] and [O I]/[C II] ratios, we find that the [CII] emission is likely dominated by the photodominated regions (PDR), instead of by ionized gas or large-scale shocks. |
WOS关键词 | FOURIER-TRANSFORM SPECTROMETER ; H-II REGIONS ; ACTIVE GALACTIC NUCLEI ; HUBBLE-SPACE-TELESCOPE ; STAR-FORMATION HISTORY ; SOUTH-POLE TELESCOPE ; NARROW-LINE REGIONS ; EARLY-TYPE GALAXIES ; DEEP-FIELD-SOUTH ; SUBMILLIMETER GALAXIES |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
出版者 | OXFORD UNIV PRESS |
WOS记录号 | WOS:000449651400006 |
源URL | [http://libir.pmo.ac.cn/handle/332002/20863] |
专题 | 中国科学院紫金山天文台 |
通讯作者 | Zhang, Zhi-Yu; Ivison, R. J. |
作者单位 | 1.Univ Edinburgh, Inst Astron, Blackford Hill, Edinburgh EH9 3HJ, Midlothian, Scotland 2.European Southern Observ, Karl Schwarzschild Str 2, D-85748 Garching, Germany 3.Chinese Acad Sci, Yunnan Observ, Kunming 650011, Yunnan, Peoples R China 4.Chinese Acad Sci, Key Lab Struct & Evolut Celestial Objects, Kunming 650011, Yunnan, Peoples R China 5.Chinese Acad Sci, Ctr Astron Mega Sci, 20A Datun Rd, Beijing 100012, Peoples R China 6.Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, S Glam, Wales 7.Max Planck Inst Extraterr Phys MPE, Giessenbachstr, D-85748 Garching, Germany 8.MPIA, Koenigstuhl 17, D-69117 Heidelberg, Germany 9.Purple Mt Observ, 2 West Beijing Rd, Nanjing 230000, Jiangsu, Peoples R China 10.Univ Lethbridge, Dept Phys, Lethbridge, AB T1K 3M4, Canada |
推荐引用方式 GB/T 7714 | Zhang, Zhi-Yu,Ivison, R. J.,George, R. D.,et al. Far-infrared Herschel SPIRE spectroscopy of lensed starbursts reveals physical conditions of ionized gas[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2018,481(1):59-97. |
APA | Zhang, Zhi-Yu.,Ivison, R. J..,George, R. D..,Zhao, Yinghe.,Dunne, L..,...&van der Werf, Paul.(2018).Far-infrared Herschel SPIRE spectroscopy of lensed starbursts reveals physical conditions of ionized gas.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,481(1),59-97. |
MLA | Zhang, Zhi-Yu,et al."Far-infrared Herschel SPIRE spectroscopy of lensed starbursts reveals physical conditions of ionized gas".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 481.1(2018):59-97. |
入库方式: OAI收割
来源:紫金山天文台
其他版本
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。