Core condensation in heavy halos: a two-stage theory for galaxy formation and clustering
Simon D. M. White,Martin J. Rees +1 more
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This article is published in Monthly Notices of the Royal Astronomical Society.The article was published on 1978-07-01 and is currently open access. It has received 3633 citations till now. The article focuses on the topics: Interacting galaxy & Protogalaxy.read more
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The Origin of the Mass-Metallicity Relation: Insights from 53,000 Star-forming Galaxies in the Sloan Digital Sky Survey
Christy Tremonti,Christy Tremonti,Timothy M. Heckman,Guinevere Kauffmann,Jarle Brinchmann,Stephane Charlot,Simon D. M. White,Mark Seibert,Mark Seibert,Eric W. Peng,Eric W. Peng,David J. Schlegel,Alan Uomoto,Alan Uomoto,Masataka Fukugita,Jon Brinkmann +15 more
TL;DR: In this paper, the relation between stellar mass and gas-phase metallicity was studied using the Sloan Digital Sky Survey imaging and spectroscopy of ~53,000 star-forming galaxies at z = 0.1.
Journal ArticleDOI
Cosmic Star-Formation History
Piero Madau,Mark Dickinson +1 more
TL;DR: In this article, the authors review the range of complementary techniques and theoretical tools that allow astronomers to map the cosmic history of star formation, heavy element production, and reionization of the Universe from the cosmic "dark ages" to the present epoch.
Journal ArticleDOI
Dark Matter Substructure within Galactic Halos
Ben Moore,Sebastiano Ghigna,Fabio Governato,George Lake,Thomas R. Quinn,Joachim Stadel,Paolo Tozzi +6 more
TL;DR: In this article, the substructure clumps are on orbits that take a large fraction of them through the stellar disk, leading to significant resonant and impulsive heating, and the model predicts that the virialized extent of the Milky Way's halo should contain about 500 satellites with circular velocities larger than the Draco and Ursa Minor systems, i.e., bound masses 108 M☉ and tidally limited sizes 1 kpc.
Journal ArticleDOI
Breaking the hierarchy of galaxy formation
Richard G. Bower,Andrew J. Benson,Rowena K. Malbon,John C. Helly,Carlos S. Frenk,Carlton M. Baugh,Shaun Cole,Cedric G. Lacey +7 more
TL;DR: In this paper, a new implementation of the Durham semi-analytic model of galaxy formation in which feedback due to active galactic nuclei (AGN) is assumed to quench cooling flows in massive halos is discussed.