Lights in the Shadows, 3D-modelling knots with MOCASSIN

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dc.creatorMorisset, C.
dc.creatorErcolano, B.
dc.date2003-10-08
dc.date.accessioned2026-07-07T02:10:16Z
dc.date.available2026-07-07T02:10:16Z
dc.descriptionMost of the enveloppes of Planetary Nebulae (and other objects like novae) are far from beeing homogeneous: clumps, knots and tails are often observed. We present here the first attempt to build a 3D-photoionization model of a knot and the corresponding tail, ionized by diffused radiation issuing from surrounding material.
dc.descriptionAsymmetric Planetary Nebulae III, ASP Conf. serie, 2004
dc.identifierhttps://arxiv.org/abs/astro-ph/0310239
dc.identifierhttp://arxiv.org/abs/astro-ph/0310239
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6683
dc.subjectAstrophysics
dc.titleLights in the Shadows, 3D-modelling knots with MOCASSIN
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