A kinematical analysis of NGC 2992
Astrophysics
2007-05-23 v1
Abstract
We present long slit spectroscopy for the [OIII] and H wavelength ranges along nine different position angles for the Sa Seyfert 1.9 galaxy NGC 2992. Double profiles are present in several regions, suggesting that the gas is not simply following galaxy rotation. A simple kinematical model, which takes into account circular rotation together with a constant radial outflow, seems to be a good approximation to account for the observed kinematics.
Keywords
Cite
@article{arxiv.astro-ph/9802029,
title = {A kinematical analysis of NGC 2992},
author = {I. Marquez and C. Boisson and F. Durret and P. Petitjean},
journal= {arXiv preprint arXiv:astro-ph/9802029},
year = {2007}
}
Comments
Accepted for publication in Astronomy & Astrophysics