Formation and evolution of bulges

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dc.creatorAthanassoula, E.
dc.creatorMartinez-Valpuesta, I.
dc.date2007-10-08
dc.date.accessioned2026-07-07T08:34:44Z
dc.date.available2026-07-07T08:34:44Z
dc.descriptionAfter presenting three ways of defining a bulge component in disc galaxies, we introduce the various types of bulges, namely the classical bulges, the boxy/peanut bulges and the disc-like bulges. We then discuss three specific topics linked to bulge formation and evolution, namely the coupled time evolution of the bar, buckling and peanut strengths; the effect of velocity anisotropy on peanut formation; and bulge formation via bar destruction.
dc.description8 pages, 3 figures, to appear in the Proceedings of the conference `Pathways through an Eclectic Universe', J.H. Knapen, T.J. Mahoney, and A. Vazdekis eds., ASP Conf. Series, 2007
dc.identifierhttps://arxiv.org/abs/0710.1518
dc.identifierhttp://arxiv.org/abs/0710.1518
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/139540
dc.subjectAstrophysics
dc.titleFormation and evolution of bulges
dc.typetext

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