Titlebook: Galactic Bulges; Eija Laurikainen,Reynier Peletier,Dimitri Gadotti Book 2016 Springer International Publishing Switzerland 2016 Dark Matte

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Bulge Growth Through Disc Instabilities in High-Redshift Galaxiesave long been studied in the low-redshift nearby Universe. There it has long been probed observationally, in particular through peanut-shaped bulges (Chap. .). This secular growth of bulges in modern disc galaxies is driven by weak, non-axisymmetric instabilities: it mostly produces pseudobulges at

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Observed Properties of Boxy/Peanut/Barlens Bulgesn), or stellar populations (old), are similar to those observed in the Milky Way. Cool central discs are often embedded in the B/P/barlens bulges. Barred galaxies contain also dynamically hot classical bulges, but it is not yet clear to what extent they are really dynamically distinct structure comp

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The Milky Way Bulge: Observed Properties and a Comparison to External Galaxieserstand their origin. The investigation of both detailed and global properties of the bulge now provide us with the opportunity to characterize the bulge as observed in models, and to place the mixed component bulge scenario in the general context of external galaxies. When writing this review, we c

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Bulge Formation via Mergers in Cosmological Simulationsies. After reviewing the results of relevant research that has been published to date, we use cosmological simulations to explore the ability of feedback to reduce or even prevent bulge growth during mergers. In dwarf galaxies, mergers actually reduce the central concentration of galaxies as the ind

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