Unravelling the origins of S0 galaxies using maximum likelihood analysis of planetary nebulae kinematics
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Sloshing in its cD halo: MUSE kinematics of the central galaxy NGC 3311 in the Hydra I clusterThe transformation of Spirals into S0 galaxies in the cluster environmentThe SLUGGS survey: chromodynamical modelling of the lenticular galaxy NGC 1023The nature of faint fuzzies from the kinematics of NGC 1023The Planetary Nebula Spectrograph survey of S0 galaxy kinematicsA SLUGGS and Gemini/GMOS combined study of the elliptical galaxy M60: wide-field photometry and kinematics of the globular cluster system
P2860
Unravelling the origins of S0 galaxies using maximum likelihood analysis of planetary nebulae kinematics
description
article
@en
im März 2011 veröffentlichter wissenschaftlicher Artikel
@de
wetenschappelijk artikel
@nl
наукова стаття, опублікована в березні 2011
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name
Unravelling the origins of S0 ...... f planetary nebulae kinematics
@en
Unravelling the origins of S0 ...... f planetary nebulae kinematics
@nl
type
label
Unravelling the origins of S0 ...... f planetary nebulae kinematics
@en
Unravelling the origins of S0 ...... f planetary nebulae kinematics
@nl
prefLabel
Unravelling the origins of S0 ...... f planetary nebulae kinematics
@en
Unravelling the origins of S0 ...... f planetary nebulae kinematics
@nl
P2093
P2860
P50
P1476
Unravelling the origins of S0 ...... f planetary nebulae kinematics
@en
P2093
A. J. Romanowsky
I. Martinez-Valpuesta
K. C. Freeman
M. Capaccioli
M. R. Merrifield
N. G. Douglas
N. R. Napolitano
O. Gerhard
P2860
P304
P356
10.1111/J.1365-2966.2011.18429.X
P407
P577
2011-03-24T00:00:00Z
P818
P819
2011MNRAS.414..642C