The low density and magnetization of a massive galaxy halo exposed by a fast radio burst

The low density and magnetization of a massive galaxy halo exposed by a fast radio burst

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...

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Bibliographic Details
Main Authors: Prochaska, J.X., Macquart, Jean-Pierre, McQuinn, M., Simha, S., Shannon, Ryan, Day, C.K., Marnoch, L., Ryder, S., Deller, A., Bannister, K.W., Bhandari, S., Bordoloi, R., Bunton, J., Cho, H., Flynn, C., Mahony, E.K., Phillips, C., Qiu, H., Tejos, N.
Format: Journal Article
Language:English
Published: AMER ASSOC ADVANCEMENT SCIENCE 2019
Subjects:
Science & Technology
Multidisciplinary Sciences
Science & Technology - Other Topics
CIRCUMGALACTIC MEDIUM
HOST GALAXY
TURBULENCE
IMPACT
CONSTRAINTS
INSTABILITY
EFFICIENT
EMISSION
SOFTWARE
REDSHIFT
astro-ph.GA
Online Access:https://www.science.org/cms/asset/6eb21dd9-e7c2-46c2-b304-7a7752c9c363/pap.pdf
http://hdl.handle.net/20.500.11937/91001

Internet

https://www.science.org/cms/asset/6eb21dd9-e7c2-46c2-b304-7a7752c9c363/pap.pdf
http://hdl.handle.net/20.500.11937/91001

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