J. S Rechy-García, Miriam Peña, \and Jorge García-Rojas
Published 2011-09-23Version 1
High resolution spectroscopic data of a large sample of galactic planetary nebulae with [WC] central stars ([WC]PNe) are analyzed to determine their kinematical behavior. Their heliocentric velocities have been determined with a precision better than a few km/s. Distances obtained from the literature are used to derive the peculiar velocities of the objects.
Comments: Poster contribution (2 pages, 1 figure) to IAU Symposium 283: "Planetary Nebulae: An Eye to the Future" held in Puerto de la Cruz, Tenerife, Spain in July 25th-29th 2011
The kinematical behavior of ORLs and CELs in PNe with [WC] central star
Galactic kinematics of planetary nebulae with [WC] central star
The kinematical behaviour of ORLs and CELs in Galactic PNe
![QR code for arXiv:1109.5162 [astro-ph.GA]](http://oss.arxitics.com/images/favicon.svg)