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DOI | 10.1126/science.aay0073 |
The low density and magnetization of a massive galaxy halo exposed by a fast radio burst | |
Prochaska, J. Xavier1,2; Macquart, Jean-Pierre3; McQuinn, Matthew4; Simha, Sunil1; Shannon, Ryan M.5; Day, Cherie K.5,6; Marnoch, Lachlan6,7; Ryder, Stuart7; Deller, Adam5; Bannister, Keith W.6; Bhandari, Shivani6; Bordoloi, Rongmon8; Bunton, John6; Cho, Hyerin9; Flynn, Chris5; Mahony, Elizabeth K.6; Phillips, Chris6; Qiu, Hao10; Tejos, Nicolas11 | |
2019-10-11 | |
发表期刊 | SCIENCE
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ISSN | 0036-8075 |
EISSN | 1095-9203 |
出版年 | 2019 |
卷号 | 366期号:6462页码:231-+ |
文章类型 | Article |
语种 | 英语 |
国家 | USA; Japan; Australia; South Korea; Chile |
英文摘要 | Present-day galaxies are surrounded by cool and enriched halo gas extending for hundreds of kiloparsecs. This halo gas is thought to be the dominant reservoir of material available to fuel future star formation, but direct constraints on its mass and physical properties have been difficult to obtain. We report the detection of a fast radio burst (FRB 181112), localized with arcsecond precision, that passes through the halo of a foreground galaxy. Analysis of the burst shows that the halo gas has low net magnetization and turbulence. Our results imply predominantly diffuse gas in massive galactic halos, even those hosting active supermassive black holes, contrary to some previous results. |
领域 | 地球科学 ; 气候变化 ; 资源环境 |
收录类别 | SCI-E |
WOS记录号 | WOS:000490014700041 |
WOS关键词 | CIRCUMGALACTIC MEDIUM ; HOST GALAXY ; TURBULENCE ; IMPACT ; CONSTRAINTS ; INSTABILITY ; EFFICIENT ; EMISSION ; SOFTWARE ; REDSHIFT |
WOS类目 | Multidisciplinary Sciences |
WOS研究方向 | Science & Technology - Other Topics |
引用统计 | |
文献类型 | 期刊论文 |
条目标识符 | http://119.78.100.173/C666/handle/2XK7JSWQ/202526 |
专题 | 地球科学 资源环境科学 气候变化 |
作者单位 | 1.Univ Calif Santa Cruz, Univ Calif Observ, Lick Observ, Santa Cruz, CA 95064 USA; 2.Kavli Inst Phys & Math Universe, 5-1-5 Kashiwanoha, Kashiwa, Chiba 2778583, Japan; 3.Curtin Univ, Int Ctr Radio Astron Res, Bentley, WA 6102, Australia; 4.Univ Washington, Dept Astron, Seattle, WA 98195 USA; 5.Swinburne Univ Technol, Ctr Astrophys & Supercomp, Hawthorn, Vic 3122, Australia; 6.Australia Telescope Natl Facil, Commonwealth Sci & Ind Res Org, POB 76, Epping, NSW 1710, Australia; 7.Macquarie Univ, Dept Phys & Astron, N Ryde, NSW 2109, Australia; 8.North Carolina State Univ, Dept Phys, Raleigh, NC 27695 USA; 9.Gwangju Inst Sci & Technol, Sch Phys & Chem, Gwangju 61005, South Korea; 10.Univ Sydney, Sch Phys, Sydney Inst Astron, Sydney, NSW 2006, Australia; 11.Pontificia Univ Catolica Valparaiso, Inst Fis, Valparaiso 4059, Chile |
推荐引用方式 GB/T 7714 | Prochaska, J. Xavier,Macquart, Jean-Pierre,McQuinn, Matthew,et al. The low density and magnetization of a massive galaxy halo exposed by a fast radio burst[J]. SCIENCE,2019,366(6462):231-+. |
APA | Prochaska, J. Xavier.,Macquart, Jean-Pierre.,McQuinn, Matthew.,Simha, Sunil.,Shannon, Ryan M..,...&Tejos, Nicolas.(2019).The low density and magnetization of a massive galaxy halo exposed by a fast radio burst.SCIENCE,366(6462),231-+. |
MLA | Prochaska, J. Xavier,et al."The low density and magnetization of a massive galaxy halo exposed by a fast radio burst".SCIENCE 366.6462(2019):231-+. |
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