English   español  
Please use this identifier to cite or link to this item: http://hdl.handle.net/10261/75137
logo share SHARE logo core CORE   Add this article to your Mendeley library MendeleyBASE

Visualizar otros formatos: MARC | Dublin Core | RDF | ORE | MODS | METS | DIDL
Exportar a otros formatos:


Growth of galactic bulges by mergers - II. Low-density satellites

AuthorsEliche-Moral, M. C.; Balcells, Marc; Aguerri, J. A. L.; González-García, A. César
Keywordsgalaxies: evolution
galaxies: interactions
galaxies: kinematics and dynamics
galaxies: nuclei
galaxies: structure
methods: N-body simulations
Instituto de Ciencias del Patrimonio
Institute of Heritage Sciences
Issue Date2006
PublisherEDP Sciences
CitationAstronomy & Astrophysics, 457 (1): 91-108.
Abstract[EN]Context. Satellite accretion events have been invoked for mimicking the internal secular evolutionary processes of bulge growth. However, N-body simulations of satellite accretions have paid little attention to the evolution of bulge photometric parameters, to the processes driving this evolution, and to the consistency of this evolution with observations. Aims. We want to investigate whether satellite accretions indeed drive the growth of bulges, and whether they are consistent with global scaling relations of bulges and discs. Methods. We perform N-body models of the accretion of satellites onto disc galaxies. A Tully-Fisher (M ∝ Vα TF rot ) scaling between primary and satellite ensures that density ratios, critical to the outcome of the accretion, are realistic. We carry out a full structural, kinematic and dynamical analysis of the evolution of the bulge mass, bulge central concentration, and bulge-to-disc scaling relations. Results. The remnants of the accretion have bulge-disc structure. Both the bulge-to-disc ratio (B/D) and the Sérsic index (n) of the remnant bulge increase as a result of the accretion, with moderate final bulge Sérsic indices: n = 1.0 to 1.9. Bulge growth occurs no matter the fate of the secondary, which fully disrupts for αTF = 3 and partially survives to the remnant center for αTF = 3.5 or 4. Global structural parameters evolve following trends similar to observations. We show that the dominant mechanism for bulge growth is the inward flow of material from the disc to the bulge region during the satellite decay. Conclusions. The models confirm that the growth of the bulge out of disc material, a central ingredient of secular evolution models,may be triggered externally through satellite accretion.
Publisher version (URL)http://dx.doi.org/10.1051/0004-6361:20065394
Appears in Collections:(INCIPIT) Artículos
Show full item record
Review this work

Related articles:

WARNING: Items in Digital.CSIC are protected by copyright, with all rights reserved, unless otherwise indicated.