2022AJ....163...69B

Query : 2022AJ....163...69B

2022AJ....163...69B - Astron. J., 163, 69-69 (2022/February-0)

Characterizing the fast radio burst host galaxy population and its connection to transients in the local and extragalactic universe.

BHANDARI S., HEINTZ K.E., AGGARWAL K., MARNOCH L., DAY C.K., SYDNOR J., BURKE-SPOLAOR S., LAW C.J., PROCHASKA J.X., TEJOS N., BANNISTER K.W., BUTLER B.J., DELLER A.T., EKERS R.D., FLYNN C., FONG W.-F., JAMES C.W., LAZIO T.J.W., LUO R., MAHONY E.K., RYDER S.D., SADLER E.M., SHANNON R.M., HAN J., LEE K. and ZHANG B.

Abstract (from CDS):

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.

Abstract Copyright: © 2022. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Galaxies - Radio interferometry - Radio bursts

Simbad objects: 33

goto Full paper

goto View the references in ADS

Number of rows : 33
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 M 31 AGN 00 42 44.330 +41 16 07.50 4.86 4.36 3.44     ~ 13622 1
2 FRB 20180916B rB 01 58 00.750 +65 43 00.30           ~ 457 0
3 NGC 821 AG? 02 08 21.1358498040 +10 59 41.832436704   12.210 11.310 10.739 9.744 ~ 592 0
4 DES J033358.99-140459.2 G 03 33 59.00 -14 04 59.5           ~ 3 0
5 FRB 200906 rB 03 33 59.08 -14 04 59.5           ~ 43 0
6 FRB 20190614D rB 04 20 18.13 +73 42 24.3           ~ 37 0
7 FRB 20201124A rB 05 07 57.600 +26 11 24.00           ~ 307 0
8 FRB 20181119D rB 05 31 58.6980 +33 08 52.588           ~ 933 0
9 ICRF J054236.1+495107 Sy1 05 42 36.13789710 +49 51 07.2337139   18.45 17.80 17.210   ~ 1573 1
10 FRB 180301 rB 06 12 43.40 +04 33 44.8           ~ 125 0
11 PSO J093.2268+04.6703 G 06 12 54.539782 +04 40 11.06238           ~ 4 0
12 M 81 Sy2 09 55 33.1726556496 +69 03 55.062505368   7.89 6.94     ~ 4725 3
13 [PR95] 30244 GlC 09 57 54.902 +68 49 00.44   20.53 19.76     ~ 12 0
14 FRB 20200120E rB 09 57 56.7 +68 49 32           ~ 219 0
15 NAME COSMOS Field reg 10 00 28.60 +02 12 21.0           ~ 3639 0
16 FRB 190714 rB 12 15 55.1 -13 01 16           ~ 64 0
17 NGC 4278 LIN 12 20 06.8242 +29 16 50.722 11.54 11.09 10.16     ~ 988 2
18 FRB 190523 rB 13 48 15.6 +72 28 11           ~ 109 0
19 FRB 200430 rB 15 18 49.54 +12 22 36.8           ~ 59 0
20 NAME Sgr 1935+2154 * 19 34 55.68 +21 53 48.2           ~ 820 1
21 FRB 190611 rB 21 22 58.91 -79 23 51.3           ~ 82 0
22 FRB 190102 rB 21 29 39.76 -79 28 32.5           ~ 83 0
23 FRB 191001 rB 21 33 24.373 -54 44 51.40           ~ 64 0
24 FRB 180924 rB 21 44 25.255 -40 54 00.10           ~ 140 0
25 FRB 181112 rB 21 49 23.630 -52 58 15.39           ~ 131 0
26 FRB 20190711A rB 21 57 40.7 -80 21 29           ~ 114 0
27 FRB 171020 rB 22 15.0 -19 40           ~ 54 0
28 FRB 190608 rB 22 16 04.74 -07 53 53.6           ~ 102 0
29 IC 1459 rG 22 57 10.60682195 -36 27 43.9966421   10.96 11.85 9.34 10.3 ~ 652 2
30 * alf PsA PM* 22 57 39.04625 -29 37 20.0533 1.31 1.25 1.16 1.11 1.09 A4V 1303 3
31 FRB 191228 rB 22 57 43.30 -29 35 38.7           ~ 37 0
32 QSO B2255-2814 Bla 22 58 05.96287687 -27 58 21.2567572   17.34 16.77 17.20   ~ 397 1
33 [VV2006] J233954.5-331018 Bla 23 39 54.53514547 -33 10 16.8813229     22.50 20.8   ~ 47 1

To bookmark this query, right click on this link: simbad:objects in 2022AJ....163...69B and select 'bookmark this link' or equivalent in the popup menu