Astronomy and Astrophysics – Astrophysics
Scientific paper
2008-10-29
Astrophysics and space science library (ASSL) vol. 319. Dordrecht: Kluwer Academic Publishers, 2004, p.723
Astronomy and Astrophysics
Astrophysics
5 pages from the proceedings of the 2004 conference "Penetrating bars through masks of cosmic dust: the Hubble tuning fork str
Scientific paper
The near orthogonal distributions of dwarf elliptical (dE) and giant elliptical (E) galaxies in the mu_e-Mag and mu_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 those between central surface brightness (mu_0) and (i) galaxy magnitude and (ii) light-profile shape (n) - suggest a similar, governing formation mechanism. Here we explain how these latter two linear trends necessitate a different behavior for dE and E galaxies, exactly as observed, in diagrams involving mu_e (and also
Graham Alister W.
Guzman Rafael
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