Characterizing the Fast Radio Burst Host Galaxy Population and its Connection to Transients in the Local and Extragalactic Universe

被引：151

作者：

Bhandari, Shivani ^{[1
]}

Heintz, Kasper E. ^{[2
,3
]}

Aggarwal, Kshitij ^{[4
,5
]}

Marnoch, Lachlan ^{[1
,6
,7
]}

Day, Cherie K. ^{[1
,8
]}

Sydnor, Jessica ^{[4
,5
]}

Burke-Spolaor, Sarah ^{[4
,5
,9
]}

Law, Casey J. ^{[10
,11
]}

Prochaska, J. Xavier ^{[12
,13
]}

Tejos, Nicolas ^{[14
]}

Bannister, Keith W. ^{[1
]}

Butler, Bryan J. ^{[15
]}

Deller, Adam T. ^{[8
]}

Ekers, R. D. ^{[1
]}

Flynn, Chris ^{[8
]}

Fong, Wen-fai ^{[16
,17
]}

James, Clancy W. ^{[18
]}

Lazio, T. Joseph W. ^{[19
]}

Luo, Rui ^{[1
]}

Mahony, Elizabeth K. ^{[1
]}

Ryder, Stuart D. ^{[6
,7
]}

Sadler, Elaine M. ^{[1
,20
]}

Shannon, Ryan M. ^{[8
]}

Han, Jinlin ^{[21
,22
,23
]}

Lee, Kejia ^{[21
,24
]}

Zhang, Bing ^{[25
]}

机构：

[1] CSIRO, Space & Astron, POB 76, Epping, NSW 1710, Australia

[2] Univ Iceland, Ctr Astrophys & Cosmol, Sci Inst, Dunhagi 5, IS-107 Reykjavik, Iceland

[3] Univ Copenhagen, Cosm Dawn Ctr DAWN, Niels Bohr Inst, Jagtvej 128, DK-2100 Copenhagen O, Denmark

[4] West Virginia Univ, Dept Phys & Astron, POB 6315, Morgantown, WV 26506 USA

[5] West Virginia Univ, Ctr Gravitat Waves & Cosmol, Chestnut Ridge Res Bldg, Morgantown, WV 26505 USA

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

[7] Macquarie Univ, Astron Astrophys & Astrophoton Res Ctr, Sydney, NSW 2109, Australia

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

[9] Canadian Inst Adv Res, MaRS Ctr West Tower,661 Univ Ave Suite 505, Toronto, ON M5G 1M1, Canada

[10] Cahill Ctr Astron & Astrophys, MC 249-17 CALTECH, Pasadena, CA 91125 USA

[11] CALTECH, Owens Valley Radio Observ, 100 Leighton Lane, Big Pine, CA 93513 USA

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

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

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

[15] Natl Radio Astron Observ, Socorro, NM 87801 USA

[16] Northwestern Univ, Ctr Interdisciplinary Explorat & Res Astrophys CI, Evanston, IL 60208 USA

[17] Northwestern Univ, Dept Phys & Astron, Evanston, IL 60208 USA

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

[19] CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91109 USA

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

[21] Chinese Acad Sci, Natl Astron Observ, 20A Datun Rd, Beijing 100012, Peoples R China

[22] Chinese Acad Sci, NAOC, CAS Key Lab FAST, Beijing 100101, Peoples R China

[23] Univ Chinese Acad Sci, Sch Astron, Beijing 100049, Peoples R China

[24] Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China

[25] Univ Nevada, Dept Phys & Astron, Las Vegas, NV 89154 USA

来源：

ASTRONOMICAL JOURNAL | 2022年 / 163卷 / 02期

基金：

美国国家科学基金会; 澳大利亚研究理事会; 美国国家航空航天局;

关键词：

GLOBULAR-CLUSTER SYSTEM; STELLAR MASS FUNCTION; GAMMA-RAY BURSTS; STAR-FORMATION; FRB; 121102; IA SUPERNOVAE; REAL-TIME; ENVIRONMENT; EVOLUTION; DISTRIBUTIONS;

D O I：

10.3847/1538-3881/ac3aec

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present the localization and host galaxies of one repeating and two apparently nonrepeating fast radio bursts (FRBs). FRB 20180301A was detected and localized with the Karl G. Jansky Very Large Array to a star-forming galaxy at z = 0.3304. FRB20191228A and FRB20200906A were detected and localized by the Australian Square Kilometre Array Pathfinder to host galaxies at z = 0.2430 and z = 0.3688, respectively. We combine these with 13 other well-localized FRBs in the literature, and analyze the host galaxy properties. We find no significant differences in the host properties of repeating and apparently nonrepeating FRBs. FRB hosts are moderately star forming, with masses slightly offset from the star-forming main sequence. Star formation and low-ionization nuclear emission-line region emission are major sources of ionization in FRB host galaxies, with the former dominant in repeating FRB hosts. FRB hosts do not track stellar mass and star formation as seen in field galaxies (more than 95% confidence). FRBs are rare in massive red galaxies, suggesting that progenitor formation channels are not solely dominated by delayed channels which lag star formation by gigayears. The global properties of FRB hosts are indistinguishable from core-collapse supernovae and short gamma-ray bursts hosts, and the spatial offset (from galaxy centers) of FRBs is mostly inconsistent with that of the Galactic neutron star population (95% confidence). The spatial offsets of FRBs (normalized to the galaxy effective radius) also differ from those of globular clusters in late- and early-type galaxies with 95% confidence.

引用

页数：20

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