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Early-type Galaxy Halo Dynamics inferred using the PN Spectrograph

Published online by Cambridge University Press:  26 May 2016

N. G. Douglas ,
A. J. Romanowsky ,
K. Kuijken ,
M. R. Merrifield ,
N. R. Napolitano ,
M. Arnaboldi ,
K. C. Freeman ,
M. Capaccioli  and
O. Gerhard
N. G. Douglas
Affiliation:
Kapteyn Institute, Groningen
A. J. Romanowsky
Affiliation:
School of Physics & Astronomy, University of Nottingham
K. Kuijken
Affiliation:
Kapteyn Institute, Groningen University of Leiden
M. R. Merrifield
Affiliation:
School of Physics & Astronomy, University of Nottingham
N. R. Napolitano
Affiliation:
Kapteyn Institute, Groningen
M. Arnaboldi
Affiliation:
INAF-Osservatorio Astronomico di Pino Torinese, Turin
K. C. Freeman
Affiliation:
RSAA, Mt. Stromlo and Siding Spring Observatories
M. Capaccioli
Affiliation:
INAF-Osservatorio Astronomico di Capodimonte, Naples
O. Gerhard
Affiliation:
Astronomisches Institut, University of Basel

Abstract

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A new instrument is providing crucial data with which to probe the structure of dark halos in elliptical galaxies

Type
Part 5: Clusters and Ellipticals
Information
Symposium - International Astronomical Union , Volume 220: Dark Matter in Galaxies , 2004 , pp. 171 - 172
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

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