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
Hauptverfasser: 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
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container_end_page 68
container_issue H15
container_start_page 68
container_title Proceedings of the International Astronomical Union
container_volume 5
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
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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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