A possible hydrodynamical equivalence for astrophysical jets

dc.creatorMendoza, S.
dc.creatorHernandez, X.
dc.creatorLee, W. H.
dc.date2003-12-05
dc.date2005-06-06
dc.date.accessioned2026-07-07T06:20:13Z
dc.date.available2026-07-07T06:20:13Z
dc.descriptionThe idea of a unified model for quasars and micro-quasars has been considered for a long time, despite the different environments and physical conditions where both classes of objects reside. Here we show the existence of a simple scaling law, relating the maximum size of a jet to the properties of the gas medium into which it expands. This appears to be valid for all types of hydrodynamical jets, and can be thought of as a broad unified model. The expansion velocity of the jet and the physical properties of the surrounding gas combine in such a way that a limit to the maximum extent of jets at different scales can be obtained.
dc.description12 pages, 1 figure. Accepted for publication on Rev.Mex.Astron.Astrofis. Expanded version
dc.identifierhttps://arxiv.org/abs/astro-ph/0312181
dc.identifierhttp://arxiv.org/abs/astro-ph/0312181
dc.identifierRev.Mex.Astron.Astrofis. 41 (2005) 453-459
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/95269
dc.subjectAstrophysics
dc.titleA possible hydrodynamical equivalence for astrophysical jets
dc.typetext

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