Titlebook: Galaxy Evolution in Groups and Clusters; A JENAM 2002 Worksho Catarina Lobo,Margarida Serote Roos,Andrea Biviano Book 2003 Springer Science

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CRATE

G. R. Gandhe,V. S. Kulkarni,Y. M. Ghugaleir use as cosmological probes. BCGs form a unique galaxy population. They are located near the gravitational centre of galaxy clusters and are the most massive galaxies in the universe, being some 10 times more luminous than L. systems. Historically, BCGs have been credited with small intrinsic dis

capillaries

Rejuvenate

Raghu Prakash,Vikram Jayaram,Ashok Saxenaface brightness profiles of BCGs out to large radii is critical for understanding the processes driving their formation. The form of the profiles yields information about the current dynamical state, constrains the accretion history of these galaxies, and places limits on any radially symmetric comp

MURAL

Machi Zawidzki,?ukasz Jankowski Release (SDSS EDR) galaxies of known redshift and brighter than r=16. The bulge-to-disk (B/D) luminosity ratios can be combined with an estimate of the galaxy’s local environment to address a number of key issues that are central to our understanding of galaxy formation:

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Antimicrobial

Debark

Takehiko Ishiguro,Koji Kajimura function is not universal, but seems to be strongly dependent upon environment. In this paper we describe an automated procedure for detecting and measuring very Low Surface Brightness (LSB) features in deep CCD data. We apply this procedure to large area CCD survey fields of the Virgo cluster and

Legion

High-Tc Thin-Film Microelectronics(A0952 + 69) and Garland using HST/WFPC2 images of these galaxies. We construct a library of synthetic Colour-Magnitude Diagrams (CMDs) based on theoretical isochrones and data-derived determinations of photometric errors. These synthetic CMDs were combined linearly and ..-compared to observed photo

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