Analytical approximation for the structure of differentially rotating barotropes

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dc.creatorOdrzywolek, Andrzej
dc.date2003-06-29
dc.date.accessioned2026-07-07T02:08:53Z
dc.date.available2026-07-07T02:08:53Z
dc.descriptionApproximate analytical formula for density distribution in differentially rotating stars is derived. Any barotropic EOS and conservative rotation law can be handled with use of this method for wide range of differential rotation strength. Results are in good qualitative agreement with comparison to the other methods. Some applications are suggested and possible improvements of the formula are discussed.
dc.description10 pages, 13 figures, accepted for publication in Monthly Notices
dc.identifierhttps://arxiv.org/abs/astro-ph/0306607
dc.identifierhttp://arxiv.org/abs/astro-ph/0306607
dc.identifierMon.Not.Roy.Astron.Soc. 345 (2003) 497-505
dc.identifierdoi:10.1046/j.1365-8711.2003.06951.x
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6231
dc.subjectAstrophysics
dc.titleAnalytical approximation for the structure of differentially rotating barotropes
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