Optical integral field spectroscopy of intermediate redshift infrared bright galaxies
文献类型：期刊论文
| 作者 | Pereira-Santaella, M.1; Rigopoulou, D.1; Magdis, G. E.2; Thatte, N.1; Alonso-Herrero, A.3; Clarke, F.1; Farrah, D.4,5; Garcia-Burillo, S.6; Hogan, L.1; Morris, S.7 |
| 刊名 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
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| 出版日期 | 2019-07-01 |
| 卷号 | 486期号:4页码:5621-5645 |
| ISSN号 | 0035-8711 |
| 关键词 | galaxies: ISM -infrared: galaxies -infrared: ISM. |
| DOI | 10.1093/mnras/stz1218 |
| 英文摘要 | The extreme infrared (IR) luminosity of local luminous and ultraluminous IR galaxies (11/LIRGs; 11 < log LIR/LE:, < 12 and log LIR /L.> 12., respectively) is mainly powered by star formation processes triggered by mergers or interactions. While INLIRGs are rare locally, at z > 1, they become more common, dominate the star formation rate (SFR) density, and a fraction of them are found to be normal disc galaxies. Therefore, there must be an evolution of the mechanism triggering these intense starbursts with redshift. To investigate this evolution, we present new optical swit,r integral field spectroscopic H cx + [N n] observations of a sample of nine intermediate-z (0.2 < z < 0.4) INEIRG systems selected from Herschel 250 p.m observations. The main results are the following: (a) the ratios between the velocity dispersion and the rotation curve amplitude indicate that 10-25 per cent (1-2 of 8) might be compatible with being isolated discs, while the remaining objects are interactinghnerging systems; (b) the ratio between un-obscured and obscured SFR traced by H cz and LIR, respectively, is similar in both local and these intermediate-z Ll/LIRGs; and (c) the ratio between 250 p.im and the total IR luminosities of these intermediate-z INEIRGs is-higher than that of local INLIRGs with the same LIR, This indicates a reduced dust temperature in these intermediate-z INLIRGs. This, together with their already measured enhanced molecular gas content, suggests that the interstellar medium conditions are different in our sample of intermediate-z galaxies when compared to local II/LIRGs. |
| WOS关键词 | SPECTRAL ENERGY-DISTRIBUTIONS ; STAR-FORMATION ; SPITZER VIEW ; SAMPLE ; STARBURST ; EVOLUTION ; DUST ; GAS |
| 资助项目 | STFC[ST/N000919/1] ; STFC[ST/N002717/1] |
| WOS研究方向 | Astronomy & Astrophysics |
| 语种 | 英语 |
| 出版者 | OXFORD UNIV PRESS |
| WOS记录号 | WOS:000474908200090 |
| 资助机构 | STFC ; STFC ; STFC ; STFC ; STFC ; STFC ; STFC ; STFC |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/26981]  |
| 专题 | 中国科学院国家天文台 |
| 通讯作者 | Pereira-Santaella, M. |
| 作者单位 | 1.Univ Oxford, Dept Phys, Keble Rd, Oxford OX1 3RH, England 2.Univ Copenhagen, Niels Bohr Inst, Cosm Dawn Ctr DAWN, Juliane Maries Vej 30, DK-2100 Copenhagen, Denmark 3.CSIC, INTA, Ctr Astrobiol CAB, ESAC Campus, E-28692 Madrid, Spain 4.Univ Hawaii, Dept Phys & Astron, 2505 Correa Rd, Honolulu, HI 96822 USA 5.Univ Hawaii, Inst Astron, 2680 Woodlawn Dr, Honolulu, HI 96822 USA 6.Observ Madrid, Observ Astron Nacl OAN IGN, Alfonso XII 3, E-28014 Madrid, Spain 7.Univ British Columbia, Dept Phys & Astron, Agr Rd, Vancouver, BC V6T 1Z1, Canada 8.Chinese Acad Sci, Natl Astron Observ China, Beijing 100012, Peoples R China 9.Chinese Acad Sci, China Chile Joint Ctr Astron, Camino Observ 1515, Santiago, Chile 10.Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA |
| 推荐引用方式 GB/T 7714 | Pereira-Santaella, M.,Rigopoulou, D.,Magdis, G. E.,et al. Optical integral field spectroscopy of intermediate redshift infrared bright galaxies[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2019,486(4):5621-5645. |
| APA | Pereira-Santaella, M..,Rigopoulou, D..,Magdis, G. E..,Thatte, N..,Alonso-Herrero, A..,...&Tecza, M..(2019).Optical integral field spectroscopy of intermediate redshift infrared bright galaxies.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,486(4),5621-5645. |
| MLA | Pereira-Santaella, M.,et al."Optical integral field spectroscopy of intermediate redshift infrared bright galaxies".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 486.4(2019):5621-5645. |
入库方式： OAI收割
来源：国家天文台
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