Measuring the Alfvénic nature of the interestellar medium: velocity anisotropy revisited
The dynamics of the interstellar medium (ISM) are strongly affected by turbulence, which shows increased anisotropy in the presence of a magnetic field. We expand upon the Esquivel & Lazarian method to estimate the Alfvén Mach number using the structure function anisotropy in velocity centroid d...
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Principais autores: | , , , , |
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Formato: | article |
Idioma: | English |
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IOP SCIENCE
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Endereço do item: | https://repositorio.ufrn.br/jspui/handle/123456789/29108 |
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