The kinematical behavior of Galactic PNe with [WC] central star
Astrophysics of Galaxies
2015-05-30 v1
Abstract
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.
Keywords
Cite
@article{arxiv.1109.5162,
title = {The kinematical behavior of Galactic PNe with [WC] central star},
author = {J. S Rechy-García and Miriam Peña and \and Jorge García-Rojas},
journal= {arXiv preprint arXiv:1109.5162},
year = {2015}
}
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