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Article
The fundamental properties of early-type galaxies in the Coma Cluster
We report the results of a high quality spectral study of early-type galaxies within the Coma Cluster core. Stellar population analysis using Lick/IDS indices to break the age/metallicity degeneracy are presen...
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Chapter
The Fundamental Properties of Early-Type Galaxies in the Coma Cluster
We report the results of a high quality spectral study of early-type galaxies within the Coma Cluster core. Stellar population analysis using Lick/IDS indices to break the age/metallicity degeneracy are presen...
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Article
Environmental Effects in the Stellar Populations of Elliptical Galaxies
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Chapter and Conference Paper
Streaming Motions of Abell Clusters Within 12000 km s-1
We describe the objectives and current status of an ongoing all-sky survey of peculiar motions for 54 Abell clusters within cz = 12000 km s-1. Preliminary Fundamental Plane plots are presented for three newly-stu...
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Chapter and Conference Paper
Peculiar Motions of Clusters in the Perseus-Pisces Region
We present results of a new study of peculiar motions of 7 clusters in the Perseus—Pisces (PP) region, using the Fundamental Plane as a distance indicator. The sample is calibrated by reference to 9 additional...
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Chapter and Conference Paper
Environmental Effects in the Stellar Populations of Elliptical Galaxies
While early work successfully modelled the stellar population of elliptical galaxies as old, single-age, metal-rich systems, there is evidence that a small amount of recent (i.e. a few Gyrs ago) star formation...
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Chapter
New D — σ Results for Coma Ellipticals
We discuss D — σ results for a new sample of ellipticals in the Coma cluster. Unlike previous studies, our sample includes many ellipticals that lie well outside the cluster core. These data have been used to est...
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Chapter
The Two-Component Cluster in Centaurus
In a previous paper (Lucey et al 1980) we reported the existence of a double-peaked velocity distribution for the rich, nearby Centaurus cluster (α = 12h 46.9m, δ = −40° 57′). We have now obtained an enlarged ...
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Article
The Centaurus I cluster of galaxies — An extreme case of contamination?
Although the virial theorem is often used to calculate a system's mass from its size and velocity dispersion, there is considerable uncertainty over the result because of the problem of defining the true membe...