Kinematics of Diffuse Ionized Gas Halos
Abstract
Existing long-slit spectral data for edge-on spiral galaxies suggesting that their Diffuse Ionized Gas (DIG) halos rotate slower than their underlying disks are summarized. An attempt to characterize lagging halos using a model of purely ballistic disk-halo flow is discussed, with the result that the model fails badly for the lagging halo of NGC 891, but is somewhat more successful for NGC 5775. New two-dimensional kinematic data on the DIG halo of NGC 4302 are presented, along with a preliminary analysis of its rotation. Two-dimensional data on NGC 5775 and a preliminary analysis of its halo rotation is discussed by Heald et al. (this volume). The halo of NGC 4302 shows clear signs of lagging on its approaching side, but also strong indications of peculiar kinematics. The kinematics of the receding side are more complex.
Cite
@article{arxiv.astro-ph/0409543,
title = {Kinematics of Diffuse Ionized Gas Halos},
author = {R. J. Rand},
journal= {arXiv preprint arXiv:astro-ph/0409543},
year = {2007}
}
Comments
8 pages, 5 figures. To appear in Extraplanar Gas, ed. R. Braun, ASP, Dwingeloo June 7-11, 2004