Using the Cloudy_3D code (Morisset, this conference), we run a set of models to build a catalog of emission line profiles of PNe. The goal is to cover the main morphologies (spherical, ellipsoidal, bipolar, thin or thick shells) and to compute profiles changing the orientation of the nebula, the expansion velocity law (including or not turbulence), the position/size of the aperture. The results is a huge set of profiles and PV-diagrams that can be compared to observations as a help to derive morpho-kinematical properties of real objects
We present images and slitless spectra which were obtained in HST surveys of Planetary Nebulae (PNe)...
Part I: Asymmetry in the Planetary Nebula phaseThe morphology of the ionized, molecular, and dust co...
Context. Complex bipolar shapes can be generated either as a planetary nebula or a symbiotic system....
International audienceWe have constructed a grid of photoionization models of spherical, elliptical ...
International audienceWe present a tool, VELNEB_3D, which can be applied to the results of 1D or 3D ...
We developed a new quick pseudo-3D photoionization code based on Cloudy (G. Ferland) and IDL (RSI) t...
We describe a pseudo-3D photoionization code, NEBU_3D and its associated visualization tool, VIS_NEB...
Aims. The origin and evolution of the shapes of bipolar planetary nebulae are poorly understood. We ...
The aim of the thesis was to develop a code and pipeline for generating 3D photoionisation models of...
Aims. We present an analysis of physical conditions in planetary nebulae (PNe) in terms of collision...
Planetary nebulae (PNe) form around low to intermediate mass stars transitioning from the giant bran...
New Planetary Nebulae (PNe) were discovered through an [O III] 5007 A emission line survey in the Ga...
The majority of planetary nebulae (PNe) show axisymmetric morphologies, whose causes are not well un...
[Context] Modern instrumentation in radioastronomy constitutes a valuable tool for studying the Univ...
We search the Hubble Space Telescope (HST) Advanced Camera for Surveys and Wide Field Camera 3 broad...
We present images and slitless spectra which were obtained in HST surveys of Planetary Nebulae (PNe)...
Part I: Asymmetry in the Planetary Nebula phaseThe morphology of the ionized, molecular, and dust co...
Context. Complex bipolar shapes can be generated either as a planetary nebula or a symbiotic system....
International audienceWe have constructed a grid of photoionization models of spherical, elliptical ...
International audienceWe present a tool, VELNEB_3D, which can be applied to the results of 1D or 3D ...
We developed a new quick pseudo-3D photoionization code based on Cloudy (G. Ferland) and IDL (RSI) t...
We describe a pseudo-3D photoionization code, NEBU_3D and its associated visualization tool, VIS_NEB...
Aims. The origin and evolution of the shapes of bipolar planetary nebulae are poorly understood. We ...
The aim of the thesis was to develop a code and pipeline for generating 3D photoionisation models of...
Aims. We present an analysis of physical conditions in planetary nebulae (PNe) in terms of collision...
Planetary nebulae (PNe) form around low to intermediate mass stars transitioning from the giant bran...
New Planetary Nebulae (PNe) were discovered through an [O III] 5007 A emission line survey in the Ga...
The majority of planetary nebulae (PNe) show axisymmetric morphologies, whose causes are not well un...
[Context] Modern instrumentation in radioastronomy constitutes a valuable tool for studying the Univ...
We search the Hubble Space Telescope (HST) Advanced Camera for Surveys and Wide Field Camera 3 broad...
We present images and slitless spectra which were obtained in HST surveys of Planetary Nebulae (PNe)...
Part I: Asymmetry in the Planetary Nebula phaseThe morphology of the ionized, molecular, and dust co...
Context. Complex bipolar shapes can be generated either as a planetary nebula or a symbiotic system....