pith. sign in

arxiv: 1110.4698 · v1 · pith:IHGEBC3Lnew · submitted 2011-10-21 · 🌌 astro-ph.GA

The San Pedro M\'artir Kinematic Catalogue of Galactic Planetary Nebulae

classification 🌌 astro-ph.GA
keywords nebulaeplanetarycataloguedatagalacticartirkinematicobjects
0
0 comments X
read the original abstract

The San Pedro M\'artir kinematic catalogue of galactic planetary nebulae provides spatially resolved, long-slit Echelle spectra for about 600 planetary nebulae. The data are presented wavelength calibrated and corrected for heliocentric motion. For most objects multiple spectra have been acquired and images with accurate slit positions on the nebulae are also presented for each object. This is the most extensive and homogeneous single source of data concerning the internal kinematics of the ionized nebular material in planetary nebulae. Data can be retrieved for individual objects or selected by groups that share some common characteristics, such as by morphological classes, galactic population, binary cores, presence of fast outflows, etc. The catalogue is available through the world wide web at http://kincatpn.astrosen.unam.mx .

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. The ubiquity of turbulence in the expanding kinematics of the ionized shells of Galactic planetary nebulae

    astro-ph.GA 2026-04 unverdicted novelty 4.0

    Turbulence is ubiquitous in the ionized shells of Galactic planetary nebulae, with residual velocities transonic or slightly supersonic and larger in inner regions and [WR]-type central stars.