Further Indications Against Jet Rotation in Young Stellar Objects

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dc.creatorSoker, Noam
dc.date2007-03-18
dc.date.accessioned2026-07-07T07:52:25Z
dc.date.available2026-07-07T07:52:25Z
dc.descriptionI discuss recent observations of asymmetries in Doppler shifts across T Tauri jets, and argue that the observed asymmetric velocity shifts and gradients do not indicate jet rotation. These observations, therefor, cannot be used as a support of a magnetized disk wind. The interaction of the jets with a twisted-tilted (wrapped) accretion disk (or the variable velocity precessing model) accounts better for the observations.
dc.descriptionReply to a contrary claim made in astro-ph/0703271
dc.identifierhttps://arxiv.org/abs/astro-ph/0703474
dc.identifierhttp://arxiv.org/abs/astro-ph/0703474
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/125870
dc.subjectAstrophysics
dc.titleFurther Indications Against Jet Rotation in Young Stellar Objects
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