Journal ArticleDOI
Systematics of Bulge-to-Disk Ratios
F. Simien,G. de Vaucouleurs +1 more
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This article is published in The Astrophysical Journal.The article was published on 1986-03-01. It has received 372 citations till now. The article focuses on the topics: Absolute magnitude & Luminosity.read more
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Simulations of the formation, evolution and clustering of galaxies and quasars
Volker Springel,Simon D. M. White,Adrian Jenkins,Carlos S. Frenk,Naoki Yoshida,Liang Gao,Julio F. Navarro,Robert J. Thacker,Darren J. Croton,John C. Helly,John A. Peacock,Shaun Cole,Peter A. Thomas,Hugh M. P. Couchman,August E. Evrard,Jörg M. Colberg,Frazers Pearce +16 more
TL;DR: It is shown that baryon-induced features in the initial conditions of the Universe are reflected in distorted form in the low-redshift galaxy distribution, an effect that can be used to constrain the nature of dark energy with future generations of observational surveys of galaxies.
Journal ArticleDOI
A Fundamental Relation Between Supermassive Black Holes and Their Host Galaxies
TL;DR: The mass of supermassive black holes correlate almost perfectly with the velocity dispersions of their host bulges, Mbh ∝ σα, where α = 48 ± 05.
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Populating a cluster of galaxies - I. Results at z=0
TL;DR: In this article, the assembly of a massive rich cluster and the formation of its constituent galaxies in a flat, low-density universe is simulated, and the most accurate model follows the collapse, the star formation history and the orbital motion of all galaxies more luminous than the Fornax dwarf spheroidal, while dark halo structure is tracked consistently throughout the cluster.
Journal ArticleDOI
Hierarchical galaxy formation
TL;DR: The GALFORM model as discussed by the authors is a semi-analytic model for calculating the formation and evolution of galaxies in hierarchical clustering cosmologies, which employs a new Monte-Carlo algorithm to follow the merging evolution of dark matter halos with arbitrary mass resolution.
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The Relation between Black Hole Mass, Bulge Mass, and Near-Infrared Luminosity
TL;DR: In this article, the authors present new accurate near-infrared (NIR) spheroid (bulge) structural parameters obtained by a two-dimensional image analysis of all galaxies with a direct black hole (BH) mass determination.