A cosmic stream of atomic carbon gas connected to a massive radio galaxy at redshift 3.8
A cosmic stream of atomic carbon gas connected to a massive radio galaxy at redshift 3.8
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Publisher
Ithaca: Cornell University Library, arXiv.org
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Language
English
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Publisher
Ithaca: Cornell University Library, arXiv.org
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Contents
The growth of galaxies in the early Universe is driven by accretion of circum- and inter-galactic gas. Simulations predict that steady streams of cold gas penetrate the dark matter halos of galaxies, providing the raw material necessary to sustain star formation. We report a filamentary stream of gas that extends for 100 kiloparsecs and connects to...
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Full title
A cosmic stream of atomic carbon gas connected to a massive radio galaxy at redshift 3.8
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TN_cdi_proquest_journals_2793243964
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2793243964
Other Identifiers
E-ISSN
2331-8422
DOI
10.48550/arxiv.2303.17484
