Poster abstract details
Kinematics study of three bulge planetary nebulae.
Abstract
With the availability of high-spectral-resolution integral-field-unit spectrographs, kinematic observations of resolved planetary nebulae became possible. Data were obtained with the VLT FLAMES Giraffe spectrograph. We used Cloudy 3D which is an IDL library to compute pseudo-3D photoionization models by interpolating between several 1D Cloudy models. The Shape tool was used to facilitate the search for the best morphology.
We present a kinematic study which bases on a range of ionization from neutral to 54 eV.Three bulge planetary nebulae (M 2-4, M 2-8 and Fg 2) in using these techniques.
We present a kinematic study which bases on a range of ionization from neutral to 54 eV.Three bulge planetary nebulae (M 2-4, M 2-8 and Fg 2) in using these techniques.