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| Does a radio jet drive the massive multiphase outflow in the ultra-luminous infrared galaxy IRAS 10565+2448? | |
Su, Renzhi1,2,3 ; Mahony, Elizabeth K.3; Gu, Minfeng1; Sadler, Elaine M.3,4,5; Curran, S. J.6; Allison, James R.5,7; Yoon, Hyein4,5; Aditya, J. N. H. S.4,5; Chandola, Yogesh8; Chen, Yongjun9,10; Moss, Vanessa A.3; Wu, Zhongzu11; Shao, Xi1,2; Liu, Xiang12; Glowacki, Marcin13; Whiting, Matthew T.3; Weng, Simon4,5
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| 2023-02-01 | |
| Source Publication | Monthly Notices of the Royal Astronomical Society
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| ISSN | 0035-8711 |
| Volume | 520Issue:4Pages:5712-5723 |
| Contribution Rank | 12 |
| Abstract | We present new upgraded Giant Metrewave Radio Telescope H I 21-cm observations of the ultra-luminous infrared galaxy IRAS 10565 + 2448, previously reported to show blueshifted, broad, and shallow H I absorption indicating an outflow. Our higher spatial resolution observations have localized this blueshifted outflow, which is similar to 1.36 kpc southwest of the radio centre and has a blueshifted velocity of similar to 148 km s(-1) and a full width at half maximum of similar to 581 km s (-1). The spatial extent and kinematic properties of the H I outflow are consistent with the previously detected cold molecular outflows in IRAS 10565 + 2448, suggesting that they likely have the same driving mechanism and are tracing the same outflow. By combining the multiphase gas observations, we estimate a total outflowing mass rate of at least 140 M-? yr (-1) and a total energy loss rate of at least 8 . 9 x 10 (42) erg s(-1), where the contribution from the ionized outflow is negligible, emphasizing the importance of including both cold neutral and molecular gas when quantifying the impact of outflows. We present evidence of the presence of a radio jet and argue that this may play a role in driving the observed outflows. The modest radio luminosity L (1 . 4GHz )similar to 1 . 3 x 10 (23) W Hz(-1) of the jet in IRAS 10565 + 2448 implies that the jet contribution to driving outflows should not be ignored in low radio luminosity active galactic nuclei. |
| Keyword | ISM: jets and outflows galaxies: active galaxies: ISM radio lines: ISM supermassive black-holes active galactic nuclei fast molecular outflows h i emission star-formation cold gas spin temperature local ulirgs feedback absorption Astronomy & Astrophysics |
| Subtype | Article |
| DOI | 10.1093/mnras/stad370 |
| Indexed By | SCI |
| Language | 英语 |
| WOS ID | WOS:000943248300003 |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.xao.ac.cn/handle/45760611-7/6648 |
| Collection | 射电天文研究室_星系宇宙学研究团组 |
| Corresponding Author | Su, Renzhi |
| Affiliation | 1.Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai 200030, China; 2.University of Chinese Academy of Sciences, 19A Yuquan Road, Beijing 100049, China; 3.ATNF, CSIRO Space and Astronomy, PO Box 76, Epping, NSW 1710, Australia; 4.Sydney Institute for Astronomy, School of Physics A28, University of Sydney, North South Wales 2006, Australia; 5.ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D); 6.School of Chemical and Physical Sciences, Victoria University of Wellington, PO Box 600, Wellington 6140, New Zealand; 7.First Light Fusion Ltd, Unit 9/10 Oxford Industrial Park, Mead Road, Yarnton, Kidlington OX5 1QU, UK; 8.Purple Mountain Observatory, Chinese Academy of Sciences, No.10 Yuanhua Road, Qixia District, Nanjing 210023, China; 9.Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai 200030, China; 10.Key Laboratory for Radio Astronomy, Chinese Academy of Sciences, Nanjing 210008, China; 11.College of Physics, Guizhou University, Guiyang 550025, PR China; 12.Xinjiang Astronomical Observatory, Chinese Academy of Sciences, 150 Science 1-Street, Urumqi 830011, China; 13.International Centre for Radio Astronomy Research, Curtin University, Bentley, Western Australia 6102, Australia |
| Recommended Citation GB/T 7714 | Su, Renzhi,Mahony, Elizabeth K.,Gu, Minfeng,et al. Does a radio jet drive the massive multiphase outflow in the ultra-luminous infrared galaxy IRAS 10565+2448?[J]. Monthly Notices of the Royal Astronomical Society,2023,520(4):5712-5723. |
| APA | Su, Renzhi.,Mahony, Elizabeth K..,Gu, Minfeng.,Sadler, Elaine M..,Curran, S. J..,...&Weng, Simon.(2023).Does a radio jet drive the massive multiphase outflow in the ultra-luminous infrared galaxy IRAS 10565+2448?.Monthly Notices of the Royal Astronomical Society,520(4),5712-5723. |
| MLA | Su, Renzhi,et al."Does a radio jet drive the massive multiphase outflow in the ultra-luminous infrared galaxy IRAS 10565+2448?".Monthly Notices of the Royal Astronomical Society 520.4(2023):5712-5723. |
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| Su-2023-Does a radio（1120KB） | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | View Application Full Text | |
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