Turbulence in the Ursa Major cirrus cloud

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dc.creatorMiville-Deschenes, Marc-Antoine
dc.creatorJoncas, Gilles
dc.creatorFalgarone, Edith
dc.date1998-04-21
dc.date.accessioned2026-07-07T02:26:39Z
dc.date.available2026-07-07T02:26:39Z
dc.descriptionHigh resolution 21 cm observations of the Ursa Major cirrus revealed highly filamentary structures down to the 0.03 pc resolution. These filaments, still present in the line centroid map, show multi-Gaussian components and seem to be associated with high vorticity regions. Probability density functions of line centroid increments and structure functions were computed on the line centroid field, providing strong evidences for the presence of turbulence in the atomic gas.
dc.description5 pages, 4 figures, to be published in 'Interstellar Turbulence', Puebla, 1998, Cambridge University Press, Pepe Franco and Alberto Carraminana eds
dc.identifierhttps://arxiv.org/abs/astro-ph/9804209
dc.identifierhttp://arxiv.org/abs/astro-ph/9804209
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12359
dc.subjectAstrophysics
dc.titleTurbulence in the Ursa Major cirrus cloud
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