The Host Galaxies and Progenitors of Fast Radio Bursts Localized with the Australian Square Kilometre Array Pathfinder

被引：130

作者：

Bhandari, Shivani ^{[1
]}

Sadler, Elaine M. ^{[1
,2
]}

Prochaska, J. Xavier ^{[3
,4
]}

Simha, Sunil ^{[3
]}

Ryder, Stuart D. ^{[5
]}

Marnoch, Lachlan ^{[1
,5
]}

Bannister, Keith W. ^{[1
]}

Macquart, Jean-Pierre ^{[6
]}

Flynn, Chris ^{[7
]}

Shannon, Ryan M. ^{[7
]}

Tejos, Nicolas ^{[8
]}

Corro-Guerra, Felipe ^{[8
]}

Day, Cherie K. ^{[1
,7
]}

Deller, Adam T. ^{[7
]}

Ekers, Ron ^{[1
,6
]}

Lopez, Sebastian ^{[9
]}

Mahony, Elizabeth K. ^{[1
]}

Nunez, Consuelo ^{[8
]}

Phillips, Chris ^{[1
]}

机构：

[1] CSIRO Astron & Space Sci, Australia Telescope Natl Facil, POB 76, Epping, NSW 1710, Australia

[2] Univ Sydney, Sch Phys A28, Sydney Inst Astron, Sydney, NSW 2006, Australia

[3] Univ Calif Santa Cruz, 1156 High St, Santa Cruz, CA 95064 USA

[4] Kavli Inst Phys & Math Universe Kavli IPMU, 5-1-5 Kashiwanoha, Kashiwa, Chiba 2778583, Japan

[5] Macquarie Univ, Dept Phys & Astron, Sydney, NSW 2109, Australia

[6] Curtin Univ, Int Ctr Radio Astron Res, Bentley, WA 6102, Australia

[7] Swinburne Univ Technol, Ctr Astrophys & Supercomp, John St, Hawthorn, Vic 3122, Australia

[8] Pontificia Univ Catolica Valparaiso, Inst Fis, Casilla 4059, Valparaiso, Chile

[9] Univ Chile, Dept Astron, Casilla 36-D, Santiago, Chile

来源：

ASTROPHYSICAL JOURNAL LETTERS | 2020年 / 895卷 / 02期

基金：

澳大利亚研究理事会;

关键词：

Galaxies; Radio continuum emission; Radio bursts; Star formation; GAMMA-RAY BURSTS; POPULATION;

D O I：

10.3847/2041-8213/ab672e

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Australian SKA Pathfinder (ASKAP) telescope has started to localize fast radio bursts (FRBs) to arcsecond accuracy from the detection of a single pulse, allowing their host galaxies to be reliably identified. We discuss the global properties of the host galaxies of the first four FRBs localized by ASKAP, which lie in the redshift range 0.11 z < 0.48. All four are massive galaxies (log(M-*/M) similar to 9.4-10.4) with modest star formation rates of up to 2 M yr(-1)-very different to the host galaxy of the first repeating FRB 121102, which is a dwarf galaxy with a high specific star formation rate. The FRBs localized by ASKAP typically lie in the outskirts of their host galaxies, which appears to rule out FRB progenitor models that invoke active galactic nuclei or free-floating cosmic strings. The stellar population seen in these host galaxies also disfavors models in which all FRBs arise from young magnetars produced by superluminous supernovae, as proposed for the progenitor of FRB 121102. A range of other progenitor models (including compact-object mergers and magnetars arising from normal core-collapse supernovae) remain plausible.

引用

页数：12

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