A new method for spatially resolving the turbulence driving mixture in the ISM with application to t...
A new method for spatially resolving the turbulence driving mixture in the ISM with application to the Small Magellanic Cloud
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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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Contents
Turbulence plays a crucial role in shaping the structure of the interstellar medium. The ratio of the three-dimensional density contrast (\(\sigma_{\rho/\rho_0}\)) to the turbulent sonic Mach number (\(\mathcal{M}\)) of an isothermal, compressible gas describes the ratio of solenoidal to compressive modes in the turbulent acceleration field of the...
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Full title
A new method for spatially resolving the turbulence driving mixture in the ISM with application to the Small Magellanic Cloud
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TN_cdi_proquest_journals_2866528904
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2866528904
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E-ISSN
2331-8422
DOI
10.48550/arxiv.2309.10755
