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相关论文: The formation of the first stars and galaxies

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How did star formation begin in the universe? Some of the questions addressed at this first meeting on "The First Stars" are summarized here from a theoretical perspective, and some brief comments are made on what we may have learned so…

天体物理学 · 物理学 2009-10-31 Richard B. Larson

The first few billion years of cosmic history witnessed the rapid emergence of the most massive galaxies, yet their true space density, baryon assembly pathways, and early quenching mechanisms remain poorly constrained. Current surveys lack…

Galaxies cover a wide range of masses and star formation histories. In this review, I summarize some of the evolutionary key features of common galaxy types. At the high-mass end, very rapid, efficient early star formation is observed,…

宇宙学与河外天体物理 · 物理学 2015-05-19 Eva K. Grebel

When, and how, did the first galaxies and supermassive black holes (SMBH) form, and how did they reionization the Universe? First galaxy formation and cosmic reionization are among the last frontiers in studies of cosmic structure…

The massive First Stars (the first ones to contribute to the chemical enrichment of the Universe due to their short lifetimes) are long dead, and even though efforts to directly observe them in high redshift galaxies are underway, a step…

星系天体物理 · 物理学 2013-01-10 Gabriele Cescutti , Cristina Chiappini

The discovery of a population of young galaxies at an epoch when the universe was about one tenth of its current age has shed new light on the question of when and how galaxies formed. Within the context of popular models this is the…

天体物理学 · 物理学 2010-04-06 F. Governato , C. M. Baugh , C. S. Frenk , S. Cole , C. G. Lacey , T. Quinn , J. Stadel

It is an obvious statement that all the galaxies we see today in and around our Local Group have been forming and evolving for a significant fraction of the age of the Universe. It is not a great leap of logic to further state that the…

天体物理学 · 物理学 2007-05-23 Eline Tolstoy

Studies of nearby galaxies including the Milky Way have provided fundamental information on the evolution of structure in the Universe, the existence and nature of dark matter, the origin and evolution of galaxies, and the global features…

宇宙学与河外天体物理 · 物理学 2009-02-24 F. J. Lockman , J. Ott

A prediction of standard inflationary cosmology is that the elemental composition of the medium out of which the earliest stars and galaxies condensed consisted primarily of hydrogen and helium 4He with small admixtures of deuterium,…

天体物理学 · 物理学 2009-11-07 Martin Harwit , Marco Spaans

Over the past two decades, an avalanche of data from multiwavelength imaging and spectroscopic surveys has revolutionized our view of galaxy formation and evolution. Here we review the range of complementary techniques and theoretical tools…

宇宙学与河外天体物理 · 物理学 2015-06-18 Piero Madau , Mark Dickinson

It is generally believed that in the epoch prior to the formation of the first stars, the Universe was completely dark (the period is therefore known as the Dark Ages). Usually, the start of this epoch is placed at the photon decoupling. In…

科普物理 · 物理学 2019-05-07 Christopher Andersen , Charlotte Amalie Rosenstroem , Oleg Ruchayskiy

(Abridged) Cosmology faces three distinct challenges in the next decade. (1) The dark sector, both dark matter and dark energy, dominates the Universe. Key questions include determining the nature of both. Improved observational probes are…

天体物理学 · 物理学 2007-12-19 Richard Ellis , Joseph Silk

Since more than a century we investigate cosmic particles coming from the Universe with the aim of understanding their nature, their origin and how they are accelerated. So far, cosmic rays have provided many impressive results, giving…

高能天体物理现象 · 物理学 2016-12-30 Mariangela Settimo

A Big Bang universe consisting, before recombination, of H, D, 3He, 4He, 6Li, and 7Li ions, electrons, photons, and massless neutrinos, at closure density, with a galaxy-size perturbation spectrum but no large-scale structure, will evolve…

天体物理学 · 物理学 2007-05-23 Robert L. Kurucz

(Abridged) In these lectures aimed for non-specialists, I review progress in understanding how galaxies form and evolve. Both the star formation history and assembly of stellar mass can be empirically traced from redshifts z~6 to the…

天体物理学 · 物理学 2015-06-24 Richard S Ellis

The rate of star formation varies between galaxy types and evolves with redshift. Most stars in the universe have formed in episodes of an exceptionally high star-forming activity, commonly called a starburst. We here summarize basic…

星系天体物理 · 物理学 2020-12-24 Ivana Orlitova

Analysis of the deepest available images of the sky, obtained by the Hubble Space Telescope, reveals a large number of candidate high-redshift galaxies. A catalogue of 1,683 objects is presented, with estimated redshifts ranging from $z=0$…

天体物理学 · 物理学 2008-11-26 Kenneth M. Lanzetta , Amos Yahil , Alberto Fernandez-Soto

How stars are born from clouds of gas is a rich physics problem whose solution will inform our understanding of not just stars but also planets, galaxies, and the universe itself. Star formation is stupendously inefficient. Take the Milky…

太阳与恒星天体物理 · 物理学 2018-12-10 Christoph Federrath

If the cosmological dark matter has a component made of small primordial black holes, they may have a significant impact on the physics of the first stars and on the subsequent formation of massive black holes. Primordial black holes would…

天体物理学 · 物理学 2009-10-28 Cosimo Bambi , Douglas Spolyar , Alexander D. Dolgov , Katherine Freese , Marta Volonteri

The James Webb Space Telescope has recently detected massive, fully formed, galaxies at redshifts corresponding to few hundred million years after the Big-Bang. However, our current cosmological model cannot produce such massive systems so…

广义相对论与量子宇宙学 · 物理学 2025-11-26 Christos G. Tsagas
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