A 3D morpho-kinematic study of NGC 3132

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dc.creatorMonteiro, H.
dc.creatorMorisset, C.
dc.creatorGruenwald, R.
dc.creatorViegas, S. M.
dc.date1999-09-28
dc.date.accessioned2026-07-07T02:33:32Z
dc.date.available2026-07-07T02:33:32Z
dc.descriptionWe present a new modeling tool for planetary nebulae (PNe), based on 3D photoionization calculations. From models for two theoretical PNe, we show that the enhancement in the equatorial zone observed in several PNe is not necessarily due to a density gradient, as usually interpreted. We study the morpho-kinematic properties of the PN NGC 3132 and show that a bipolar Diabolo shape successfully reproduces the observed images, as well as the high resolution observations.
dc.description4 pages, 6 figures, to appear in ``Asymmetrical Planetary Nebulae II: from Origins to Microstructures,'' ASP Conference Series, J.H. Kastner, N. Soker, & S.A. Rappaport, eds
dc.identifierhttps://arxiv.org/abs/astro-ph/9909468
dc.identifierhttp://arxiv.org/abs/astro-ph/9909468
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/14877
dc.subjectAstrophysics
dc.titleA 3D morpho-kinematic study of NGC 3132
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