{ "id": "astro-ph/9808325", "version": "v1", "published": "1998-08-28T09:16:52.000Z", "updated": "1998-08-28T09:16:52.000Z", "title": "The Formation History of Early-Type Galaxies: An Observational Perspective", "authors": [ "Richard G. Bower", "Ale Terlevich", "Tadayuki Kodama", "Nelson Caldwell" ], "comment": "to appear in Star Formation in Early-Type Galaxies, ASP Conf. Ser., eds. P. Carral & J. Cepa; paspconf.sty LaTeX, 16 pages, 7 figures", "categories": [ "astro-ph" ], "abstract": "This talk investigates the formation of early-type galaxies from a deliberately observational view point. I begin by reviewing the conclusions that can be reached by comparing the detailed properties of galaxies in present-day clusters, focusing on the colour-magnitude relation in particular. The overriding picture is one of homogeneity, implying a remarkable uniformity in the formation of these galaxies. This picture contrasts with the increasing activity seen in clusters as a function of redshift, creating an apparent paradox been the obvious diversity of star formation histories in distant cluster galaxies and their uniformity in local systems. A resolution is feasible so long as star formation occurs over an extended epoch. In addition to placing limits on variations in star formation history the existence of a tight `fundamental relations', such as the colour-magnitude relation, can be used to investigate galaxy mergers and to set limits on the degree to which present-day clusters galaxies are built by combining systems of stars formed in smaller units. The final part of this talk turns to early-type galaxies in the field, and tries to apply the same techniques that have been successful in clusters. This is an emerging field in which appropriate data-sets are only just becoming available; however, comparison of the formation histories of galaxies in a wide variety of environments is key to distinguishing between the Classical and Hierarchical models for galaxy formation.", "revisions": [ { "version": "v1", "updated": "1998-08-28T09:16:52.000Z" } ], "analyses": { "keywords": [ "early-type galaxies", "observational perspective", "star formation history", "colour-magnitude relation", "present-day clusters galaxies" ], "note": { "typesetting": "LaTeX", "pages": 16, "language": "en", "license": "arXiv", "status": "editable", "inspire": 483372 } } }