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相关论文: Formation of the First Galaxies: Theory and Simula…

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The formation of the first galaxies at redshifts z~10-15 signaled the transition from the simple initial state of the universe to one of ever increasing complexity. We here review recent progress in understanding their assembly process with…

天体物理学 · 物理学 2009-10-20 Thomas H. Greif , Jarrett L. Johnson , Volker Bromm

The formation of the first generations of stars at redshifts z > 15-20 signaled the transition from the simple initial state of the universe to one of increasing complexity. We here review recent progress in understanding the assembly…

天体物理学 · 物理学 2009-11-13 Jarrett L. Johnson , Thomas H. Greif , Volker Bromm

Understanding the formation of the first stars and galaxies is a key problem in modern cosmology. In these lecture notes, we will derive some of the basic physical principles underlying this emerging field. We will consider the basic…

宇宙学与河外天体物理 · 物理学 2012-03-20 Volker Bromm

The primary concern of this thesis is to understand the formation and properties of the first galaxies, as well as the influence of the first stars in terms of radiative, mechanical and chemical feedback. In particular, we elucidate the…

宇宙学与河外天体物理 · 物理学 2009-05-21 Thomas H. Greif

The basic processes of the formation of the first stars in the primordial Universe are outlined and the implications for cosmological structure formation discussed. By employing theoretical and numerical models of cosmic structure evolution…

星系天体物理 · 物理学 2016-06-16 U. Maio

Galaxy formation is at the heart of our understanding of cosmic evolution. Although there is a consensus that galaxies emerged from the expanding matter background by gravitational instability of primordial fluctuations, a number of…

星系天体物理 · 物理学 2020-06-10 Pratika Dayal , Andrea Ferrara

First-generation (Population III) stars in the universe play an important role inearly enrichment of heavy elements in galaxies and intergalactic medium and thus affect the history of galaxies. The physical and chemical properties of…

Cosmic structure originated from minute density perturbations in an almost homogeneous universe. The first stars are believed to be very massive and luminous, providing the first ionizing radiation and heavy elements to the universe and…

天体物理学 · 物理学 2008-04-28 John H. Wise

The elegance of inflationary cosmology and cosmological perturbation theory ends with the formation of the first stars and galaxies, the initial sources of light that launched the phenomenologically rich process of cosmic reionization. Here…

星系天体物理 · 物理学 2016-01-27 Milos Milosavljevic , Chalence Safranek-Shrader

We review our current understanding of how the first galaxies formed at the end of the cosmic dark ages, a few 100 million years after the Big Bang. Modern large telescopes discovered galaxies at redshifts greater than seven, whereas…

宇宙学与河外天体物理 · 物理学 2015-05-27 Volker Bromm , Naoki Yoshida

In this review, I survey our current understanding of how the very first stars in the universe formed, with a focus on three main areas of interest: the formation of the first protogalaxies and the cooling of gas within them, the nature and…

天体物理学 · 物理学 2016-08-30 Simon C. O. Glover

The nature of the first generation of stars in the Universe remains largely unknown. Observations imply the existence of massive primordial stars early in the history of the universe, and the standard theory for the growth of cosmic…

天体物理学 · 物理学 2009-11-13 Naoki Yoshida , Kazuyuki Omukai , Lars Hernquist

Observations made using large ground-based and space-borne telescopes have probed cosmic history all the way from the present-day to a time when the Universe was less than a tenth of its present age. Earlier on lies the remaining frontier,…

宇宙学与河外天体物理 · 物理学 2015-05-13 Volker Bromm , Naoki Yoshida , Lars Hernquist , Christopher F. McKee

We review recent theoretical results on the formation of the first stars in the universe, and emphasize related open questions. In particular, we discuss the initial conditions for Population III star formation, as given by variants of the…

天体物理学 · 物理学 2008-11-26 Volker Bromm , Richard B. Larson

The first generation of stars was formed from primordial gas. Numerical simulations suggest that the first stars were predominantly very massive, with typical masses M > 100 Mo. These stars were responsible for the reionization of the…

太阳与恒星天体物理 · 物理学 2015-05-18 D. Bahena , J. Klapp

The formation and evolution of galaxies is one of the great outstanding problems of astrophysics. Within the broad context of hierachical structure formation, we have only a crude picture of how galaxies like our own came into existence. A…

天体物理学 · 物理学 2011-03-10 Ken Freeman , Joss Bland-Hawthorn

Using three-dimensional cosmological simulations, we study the assembly process of one of the first galaxies, with a total mass of 10^8 M_sun, collapsing at z = 10. Our main goal is to trace the transport of the heavy chemical elements…

宇宙学与河外天体物理 · 物理学 2015-05-18 Thomas H. Greif , Simon C. O. Glover , Volker Bromm , Ralf S. Klessen

Star forming galaxies represent a valuable tracer of cosmic history. Recent observational progress with Hubble Space Telescope has led to the discovery and study of the earliest-known galaxies corresponding to a period when the Universe was…

宇宙学与河外天体物理 · 物理学 2015-05-20 Brant E. Robertson , Richard S. Ellis , James S. Dunlop , Ross J. McLure , Daniel P. Stark

We review recent theoretical results on the formation of the first stars and quasars in the universe, and emphasize related open questions. In particular, we list important differences between the star formation process at high redshifts…

天体物理学 · 物理学 2009-11-07 Volker Bromm , Abraham Loeb

The first stars fundamentally transformed the early universe by emitting the first light and by producing the first heavy elements. These effects were predetermined by the mass distribution of the first stars, which is thought to have been…

宇宙学与河外天体物理 · 物理学 2015-06-03 Takashi Hosokawa , Kazuyuki Omukai , Naoki Yoshida , Harold W. Yorke
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