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On the Unification of Dwarf and Giant Elliptical Galaxies

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Penetrating Bars through Masks of Cosmic Dust

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 319))

Abstract

The near orthogonal distributions of dwarf elliptical (dE) and giant elliptical (E) galaxies in the µ e M and µ e −log R e diagrams have been interpreted as evidence for two distinct galaxy formation processes. However, continuous, linear relationships across the alleged dE/E boundary at M B = −18 mag — such as the relationships between central surface brightness (µ 0) and: a) galaxy magnitude (M); and b) light-profile shape (n) — suggest a similar initial formation mechanism. Here we explain how these latter two trends in fact necessitate a different behavior for dE and E galaxies, exactly as observed, in diagrams involving µ e (and also <µ>e). Together with other linear trends across the alleged dE/E boundary, such as those between luminosity and color, metallicity, and velocity dispersion, it appears that the dEs form a continuous extension to the E galaxies. The presence of partially depleted cores in luminous (M B < −20.5 mag) Es does however signify the action of a different physical process at the centers (<~300 pc) of these galaxies.

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© 2004 Springer Science+Business Media New York

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Graham, A.W., Guzman, R. (2004). On the Unification of Dwarf and Giant Elliptical Galaxies. In: Block, D.L., Puerari, I., Freeman, K.C., Groess, R., Block, E.K. (eds) Penetrating Bars through Masks of Cosmic Dust. Astrophysics and Space Science Library, vol 319. Springer, Dordrecht. https://doi.org/10.1007/978-1-4020-2862-5_62

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  • DOI: https://doi.org/10.1007/978-1-4020-2862-5_62

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-015-7085-5

  • Online ISBN: 978-1-4020-2862-5

  • eBook Packages: Springer Book Archive

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