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Related papers: The First Nonlinear Structures and the Reionizatio…

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The first galaxies formed at high redshifts, and were likely substantially less massive than typical galaxies in the local universe. We argue that (1) the reionization of a clumpy intergalactic medium by redshift z=6, (2) its enrichment by…

Astrophysics · Physics 2009-11-07 Zoltan Haiman

The development of primordial inhomogeneities into the non-linear regime and the formation of the first bound objects mark the transition from a simple cooling universe -- described by just a few parameters -- to a very messy hot one -- the…

Astrophysics · Physics 2009-11-07 Piero Madau

In popular cold dark matter cosmological scenarios, stars may have first appeared in significant numbers around a redshift of 10 or so, as the gas within protogalactic halos with virial temperatures in excess of 20,000 K (corresponding to…

Astrophysics · Physics 2007-05-23 Piero Madau

The development of primordial inhomogeneities into the non-linear regime and the formation of the first astrophysical objects within dark matter halos mark the transition from a simple, neutral, cooling universe -- described by just a few…

Astrophysics · Physics 2017-08-23 Piero Madau , Michael Kuhlen

One of the milestones in the cosmic history is the formation of the first luminous objects and Hydrogen reionization. The standard theory of cosmic structure formation predicts that the first generation of stars were born about a few…

Cosmology and Nongalactic Astrophysics · Physics 2014-07-02 Aravind Natarajan , Naoki Yoshida

The formation of the first stars and quasars marks the transformation of the universe from its smooth initial state to its clumpy current state. In popular cosmological models, the first sources of light began to form at redshift 30 and…

Astrophysics · Physics 2011-08-23 Rennan Barkana , Abraham Loeb

In popular cold dark matter cosmological scenarios, stars may have first appeared in significant numbers around a redshift of 10 or so, as the gas within protogalactic halos with virial temperatures in excess of 20,000 K (corresponding to…

Astrophysics · Physics 2007-05-23 Piero Madau

The Universe's dark ages end with the formation of the first generation of galaxies. These objects start emitting ultraviolet radiation that carves out ionized regions around them. After a sufficient number of ionizing sources have formed,…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-05 Saleem Zaroubi

The cosmic dark ages and the epoch of reionization, during which the first generations of stars and galaxies formed, are among the most compelling frontiers of extragalactic astrophysics and cosmology. Here we describe an exciting new probe…

The intergalactic medium was reionized before redshift z~6, most likely by starlight which escaped from early galaxies. The very first stars formed when hydrogen molecules (H2) cooled gas inside the smallest galaxies, minihalos of mass…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-05 Kyungjin Ahn , Ilian T. Iliev , Paul R. Shapiro , Garrelt Mellema , Jun Koda , Yi Mao

This work studies the connection between the first galaxies and their hosting dark matter halos in the early Universe when Reionization is concluding. Our numerical models (already presented in an earlier study) trace the star formation…

Cosmology and Nongalactic Astrophysics · Physics 2021-12-23 Luz Ángela García

The universe would have been completely dark between the epoch of recombination and the development of the first non-linear structure. But at redshifts beyond 5 -- perhaps even beyond 20 -- stars formed within `subgalaxies' and created the…

Astrophysics · Physics 2009-10-31 Martin J. Rees

The first structures in the Universe formed at z>7, at higher redshift than all currently known galaxies. Since GRBs are brighter than other cosmological sources at high redshift and exhibit simple power-law afterglow spectra that is ideal…

How and when did the first generation of stars form at the end of the cosmic dark ages? Quite generically, within variants of the cold dark matter model of cosmological structure formation, the first sources of light are expected to form in…

Astrophysics · Physics 2009-11-11 Volker Bromm

Probing the growth of structure from the epoch of hydrogen recombination to the formation of the first stars and galaxies is one of the most important uncharted areas of observational cosmology. Far-IR spectroscopy covering $\lambda$…

The formation of the first stars and quasars marks the transition between the smooth initial state and the clumpy current state of the Universe. In popular CDM cosmologies, the first sources of light started to form at a redshift z=30 and…

Astrophysics · Physics 2007-05-23 Abraham Loeb

The high ionization level and universal metallicity (1% solar) of the intergalactic gas at redshifts z<5 implies that nonlinear structure had started to form in the universe at earlier times than we currently probe. In Cold Dark Matter…

Astrophysics · Physics 2009-10-28 Zoltan Haiman , Abraham Loeb

In popular cosmological scenarios, some time beyond a redshift of 10, stars within protogalaxies created the first heavy elements; these systems, together perhaps with an early population of quasars, generated the ultraviolet radiation and…

Astrophysics · Physics 2009-10-31 Piero Madau

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…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-20 Brant E. Robertson , Richard S. Ellis , James S. Dunlop , Ross J. McLure , Daniel P. Stark

Cosmic objects with magnetic fields (quasars, radiogalaxies) are observed at redshifts $z\geq 7$ (Wang et al., 2021, Fan et al., 2023, Yang et al., 2024) and more (for instance, for $z = 10.073\pm 0.002$, Goulding et al., 2023) indicates…

Cosmology and Nongalactic Astrophysics · Physics 2024-06-06 M. Demiański , A. Doroshkevich , T. Larchenkova
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