Mixing and Transfer of Elements by Triaxiality

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dc.creatorFriedli, D.
dc.date1998-01-23
dc.date.accessioned2026-07-07T02:25:54Z
dc.date.available2026-07-07T02:25:54Z
dc.descriptionVarious large-scale processes induced by triaxial potentials and able to alter stellar and gaseous abundance profiles are reviewed. In particular, strong bars can quickly and efficiently blend stars through chaotic mixing, and entail intricate inflows/outflows of gas. Bar-generated abundance features include flattenings, breaks, and plateaus in radial gradients as well as box- or peanut-like morphologies.
dc.description8 pages with 8 figures. To be published in the proceedings of "Abundance Profiles: Diagnostic Tools for Galaxy History", ed. D. Friedli, M.G. Edmunds, C. Robert, L. Drissen, ASP Conf. Ser
dc.identifierhttps://arxiv.org/abs/astro-ph/9801231
dc.identifierhttp://arxiv.org/abs/astro-ph/9801231
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12058
dc.subjectAstrophysics
dc.titleMixing and Transfer of Elements by Triaxiality
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