Related papers: Blue E/S0 galaxies: merger remnants or disk rebuil…

This paper has been withdrawn, since it contains a corollary with impossible consequences and the source of an error is currently unknown.

This paper has been withdrawn because it is a duplicate of [hep-ph/0609266].

This paper has been withdrawn.

This paper has been withdrawn by the author, due to two identical copies of the paper.

This paper has been withdrawn. The results are now part of math.GR/9804072.

This paper has been withdrawn by the author(s), see hep-th/0205152.

This paper has been withdrawn, and will be superseded by another submission.

This paper has been withdrawn by the authors.

This paper has been withdrawn by the authors, since it has been merged with Part I (ID 0802.3570)

This paper has been withdrawn.

This paper has been withdrawn by the author, since now all four parts of the review are available as a single file 0804.1639

This paper has been withdrawn.

The paper has been withdrawn.

Recent work has identified a population of low-redshift E/S0 galaxies that lie on the blue sequence in color vs. stellar mass parameter space, where spiral galaxies typically reside. While high-mass blue-sequence E/S0s often resemble young…

This paper has been withdrawn and no version of it will ever be published.

This paper has been withdrawn by the authors due to several major changes in concepts and results. New version will follow briefly as a new e-print.

This paper has been withdrawn by the author.

This paper has been withdrawn by the author; see the much expanded, improved, and generalized version at arXiv:0811.2073.

This paper has been withdrawn by the authors.

This is the summary chapter of a review book on galaxy bulges. Bulge properties and formation histories are more varied than those of ellipticals. I emphasize two advances: 1 - "Classical bulges" are observationally indistinguishable from…