Cosmology

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Colour (approximate to age?) gradients in spiral galaxies

NEW LIGHT ON GALAXY EVOLUTION (1996) 358-358
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How many ULIRGs are mergers

IAU SYMP (1996) 354-354

Authors:

DL Clements, RG Mcmahon, WJ Sutherland, W Saunders
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Line strength gradients in low luminosity galaxies

NEW LIGHT ON GALAXY EVOLUTION (1996) 387-387

Authors:

C Halliday, G Baggley, RL Davies, M Birkinshaw, R Bender, R Saglia
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The detection of malignant masses by non-linear multiscale analysis

INT CONGR SER 1119 (1996) 335-340

Authors:

L Miller, N Ramsey

Abstract:

We report on the development of a new method for detecting automatically malignant masses in digitised mammograms, based on a novel non-linear method of multiscale analysis. We show that it is possible to detect > 85 percent of all malignant masses by this method, irrespective of their size, with a false-alarm rate that is close to acceptable for asymptomatic screening.
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The peculiar motions of early-type galaxies in two distant regions .1. Cluster and galaxy selection

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES 106:1 (1996) 1-26

Authors:

G Wegner, M Colless, G Baggley, RL Davies, E Bertschinger, D Burstein, RK McMahan, RP Saglia
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