Cooling of Pre-Galactic Gas Clouds by Hydrogen Molecule
Reads0
Chats0
About:
This article is published in Progress of Theoretical Physics.The article was published on 1969-08-01 and is currently open access. It has received 93 citations till now. The article focuses on the topics: Hydrogen & Galaxy.read more
Citations
More filters
Journal ArticleDOI
In the Beginning: The First Sources of Light and the Reionization of the Universe
Rennan Barkana,Abraham Loeb +1 more
TL;DR: The formation of the first stars and quasars marks the transformation of the universe from its smooth initial state to its clumpy current state as discussed by the authors, and the study of high-redshift sources is likely to attract major attention in observational and theoretical cosmology over the next decade.
Journal ArticleDOI
The First Stars
Volker Bromm,Richard B. Larson +1 more
TL;DR: In this paper, the authors discuss the initial conditions for Population III star formation, as given by variants of the cold dark matter cosmology, and show how complementary observations, both at high redshifts and in our local cosmic neighborhood, can be utilized to probe the first epoch of star formation.
Journal ArticleDOI
In the Beginning: The First Sources of Light and the Reionization of the Universe
Rennan Barkana,Abraham Loeb +1 more
TL;DR: The formation of the first stars and quasars marks the transformation of the universe from its smooth initial state to its clumpy current state as discussed by the authors, and the study of high-redshift sources is likely to attract major attention in observational and theoretical cosmology over the next decade.
Journal ArticleDOI
Simulations of Early Structure Formation: Primordial Gas Clouds
TL;DR: In this paper, the authors used cosmological simulations to study the origin of primordial star-forming clouds in a ΛCDM universe, by following the formation of dark matter halos and the cooling of gas within them.
Journal ArticleDOI
Formation of Primordial Stars in a ΛCDM Universe
TL;DR: In this article, the formation of the first generation of stars in the standard cold dark matter model was studied using a very high resolution cosmological hydrodynamic simulation that achieves a dynamic range of ~1010 in length scale.