Kinematic properties of early type galaxy halos using planetary nebulae
We studied the kinematics of the halo of a sample of 16 early type galaxies out to 5-10 effective radii using Planetary Nebulae (PNe) as kinematic tracers (Coccato et al. 2009).
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Veröffentlicht in: | Proceedings of the International Astronomical Union 2009-11, Vol.5 (H15), p.68-68 |
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creator | Coccato, L. Gerhard, O. Arnaboldi, M. Das, P. Douglas, N. G. Kuijken, K. Merrifield, M. R. Napolitano, N. R. Noordermeer, E. Romanowsky, A. J. Capaccioli, M. Cortesi, A. Lorenzi, F. De |
description | We studied the kinematics of the halo of a sample of 16 early type galaxies out to 5-10 effective radii using Planetary Nebulae (PNe) as kinematic tracers (Coccato et al. 2009). |
doi_str_mv | 10.1017/S1743921310008239 |
format | Article |
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subjects | Astronomy Astrophysics Contributed Papers Kinematics Nebulae Star & galaxy formation Stars & galaxies |
title | Kinematic properties of early type galaxy halos using planetary nebulae |
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