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most citedKinematic properties of early-type galaxy haloes using planetary nebulae

219 citations · 1.4k across the 17 of their papers we have counts for

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astro-ph2008★ 219 cited

Kinematic properties of early-type galaxy haloes using planetary nebulae

L. Coccato, O. Gerhard, M. Arnaboldi +11

We present new planetary nebulae (PNe) positions, radial velocities, and magnitudes for 6 early-type galaxies obtained with the Planetary Nebulae Spectrograph, their two-dimensiona…

astro-ph2008★ 2 cited

Probing the kinematics of early-type galaxy halos using planetary nebulae

L. Coccato, O. Gerhard, M. Arnaboldi +11

We present first results of a study of the halo kinematics for a sample of early type galaxies using planetary nebulae (PNe) as kinematical tracers. PNe allow to extend up to sever…

astro-ph2008★ 135 cited

The PN.S Elliptical Galaxy Survey: the dark matter in NGC 4494

N. R. Napolitano, A. J. Romanowsky, L. Coccato +12

We present new Planetary Nebula Spectrograph observations of the ordinary elliptical galaxy NGC 4494, resulting in positions and velocities of 255 PNe out to 7 effective radii (25…

astro-ph2008★ 19 cited

Exploring Disk Galaxy Dynamics Using IFU Data

E. Noordermeer, M. R. Merrifield, A. Aragon-Salamanca

In order to test the basic equations believed to dictate the dynamics of disk galaxies, we present and analyze deep two-dimensional spectral data obtained using the PPAK integral f…

astro-ph2008★ 125 cited

Dearth of dark matter or massive dark halo? Mass-shape-anisotropy degeneracies revealed by NMAGIC dynamical models of the elliptical galaxy NGC 3379

F. De Lorenzi, O. Gerhard, L. Coccato +10

Recent results from the Planetary Nebula Spectrograph (PN.S) survey have revealed a rapidly falling velocity dispersion profile in the nearby elliptical galaxy NGC 3379, casting do…

astro-ph2008★ 56 cited

The rotation curves of flattened Sersic bulges

E. Noordermeer

I present a method to deproject the observed intensity profile of an axisymmetric bulge with arbitrary flattening to derive the 3D luminosity density profile and to calculate the c…