TY - JOUR
T1 - The low density and magnetization of a massive galaxy halo exposed by a fast radio burst
AU - Prochaska, J. Xavier
AU - Macquart, Jean Pierre
AU - McQuinn, Matthew
AU - Simha, Sunil
AU - Shannon, Ryan M.
AU - Day, Cherie K.
AU - Marnoch, Lachlan
AU - Ryder, Stuart
AU - Deller, Adam
AU - Bannister, Keith W.
AU - Bhandari, Shivani
AU - Bordoloi, Rongmon
AU - Bunton, John
AU - Cho, Hyerin
AU - Flynn, Chris
AU - Mahony, Elizabeth K.
AU - Phillips, Chris
AU - Qiu, Hao
AU - Tejos, Nicolas
N1 - Publisher Copyright:
© 2019 American Association for the Advancement of Science. All rights reserved.
Copyright:
Copyright 2019 Elsevier B.V., All rights reserved.
PY - 2019/10/11
Y1 - 2019/10/11
N2 - 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.
AB - 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.
UR - http://www.scopus.com/inward/record.url?scp=85073126258&partnerID=8YFLogxK
U2 - 10.1126/science.aay0073
DO - 10.1126/science.aay0073
M3 - Article
C2 - 31558577
AN - SCOPUS:85073126258
SN - 0036-8075
VL - 366
SP - 231
EP - 234
JO - Science
JF - Science
IS - 6462
ER -