A common colour-magnitude relation from giant elliptical galaxies to globular clusters - Astrophysics > Cosmology and Nongalactic AstrophysicsReportar como inadecuado




A common colour-magnitude relation from giant elliptical galaxies to globular clusters - Astrophysics > Cosmology and Nongalactic Astrophysics - Descarga este documento en PDF. Documentación en PDF para descargar gratis. Disponible también para leer online.

Abstract: We discuss the existence of a common colour-magnitude relation CMR ofmetal-poor globular clusters and early-type galaxies, i.e. giant ellipticals,normal ellipticals and lenticulars, dwarf ellipticals and lenticulars, anddwarf spheroidals. Such CMR would cover a range of ~ 14 mag, extending from thebrightest galaxies, down to the globular clusters on the fainter side.



Autor: A.V. Smith Castelli, L. P. Bassino, T. Richtler, F. Faifer, J. C. Forte, S. A. Cellone

Fuente: https://arxiv.org/







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