Are Cosmological Gas Accretion Streams Multiphase and Turbulent?
Are Cosmological Gas Accretion Streams Multiphase and Turbulent?
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Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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Simulations of cosmological filamentary accretion reveal flows ("streams") of warm gas, ~\(10^4\) K, which are efficient in bringing gas into galaxies. We present a phenomenological scenario where gas in such flows -- if it is shocked as it enters the halo as we assume -- become biphasic and, as a result, turbulent. We consider a collimated stream...
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Are Cosmological Gas Accretion Streams Multiphase and Turbulent?
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TN_cdi_proquest_journals_2071717520
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2071717520
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E-ISSN
2331-8422
DOI
10.48550/arxiv.1609.04405
