A Connection Between Bulge Properties and the Bimodality of Galaxies
Niv Drory (1, 2), David B. Fisher (1) ((1) The University of, Texas at Austin, (2) Max-Planck Institut fuer Extraterrestrische Physik -, MPE, Garching)

TL;DR
This study shows that the bimodal color distribution of galaxies is strongly linked to the type of bulge they contain, with classical bulges associated with red galaxies and pseudobulges with blue ones, indicating different evolutionary paths.
Contribution
It demonstrates that galaxy color bimodality depends on bulge type rather than bulge prominence alone, highlighting the importance of bulge classification in galaxy evolution.
Findings
Classical bulges are in red galaxies at the same B/T ratio.
Pseudobulges are in blue galaxies at the same B/T ratio.
Bulge type predicts galaxy position in global structural parameters.
Abstract
The global colors of galaxies have recently been shown to follow bimodal distributions. Galaxies separate into a ``red sequence'', populated prototypically by early-type galaxies, and a ``blue cloud'', whose typical objects are late-type disk galaxies. Intermediate-type (Sa-Sbc) galaxies populate both regions. It has been suggested that this bimodality reflects the two-component nature of disk-bulge galaxies. However, it has now been established that there are two types of bulges: ``classical bulges'' that are dynamically hot systems resembling (little) ellipticals, and ``pseudobulges'', dynamically cold, flattened, disk-like structures that could not have formed via violent relaxation. Therefore thee question is whether at types Sa-Sbc, where both bulge types are found, the red-blue dichotomy separates galaxies at some value of disk-to-bulge ratio, , or, whether it separates…
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