scholarly journals Studying the first galaxies with ALMA

Author(s):  
C. L. Carilli ◽  
F. Walter ◽  
R. Wang ◽  
A. Wootten ◽  
K. Menten ◽  
...  
Keyword(s):  
Author(s):  
Abraham Loeb ◽  
Steven R. Furlanetto

This book provides a comprehensive, self-contained introduction to one of the most exciting frontiers in astrophysics today: the quest to understand how the oldest and most distant galaxies in our universe first formed. Until now, most research on this question has been theoretical, but the next few years will bring about a new generation of large telescopes that promise to supply a flood of data about the infant universe during its first billion years after the big bang. This book bridges the gap between theory and observation. It is an invaluable reference for students and researchers on early galaxies. The book starts from basic physical principles before moving on to more advanced material. Topics include the gravitational growth of structure, the intergalactic medium, the formation and evolution of the first stars and black holes, feedback and galaxy evolution, reionization, 21-cm cosmology, and more.


2012 ◽  
Author(s):  
Chalence Safranek-Shrader ◽  
Meghann Agarwal ◽  
Christoph Federrath ◽  
Anshu Dubey ◽  
Milos Milosavljevic ◽  
...  
Keyword(s):  
Free Gas ◽  

2015 ◽  
Vol 455 (3) ◽  
pp. 3288-3302 ◽  
Author(s):  
Chalence Safranek-Shrader ◽  
Michael H. Montgomery ◽  
Miloš Milosavljević ◽  
Volker Bromm

2010 ◽  
Author(s):  
Chalence Safranek-Shrader ◽  
Daniel J. Whalen ◽  
Volker Bromm ◽  
Naoki Yoshida
Keyword(s):  

2010 ◽  
Author(s):  
C. L. Carilli ◽  
Daniel J. Whalen ◽  
Volker Bromm ◽  
Naoki Yoshida ◽  

2010 ◽  
Author(s):  
Dominik R. G. Schleicher ◽  
Robi Banerjee ◽  
Sharanya Sur ◽  
Simon C. O. Glover ◽  
Marco Spaans ◽  
...  

Author(s):  
L. Danese ◽  
F. Shankar ◽  
G.L. Granato ◽  
L. Silva ◽  
A. Bressan ◽  
...  
Keyword(s):  

2010 ◽  
Author(s):  
Mark Dijkstra ◽  
Daniel J. Whalen ◽  
Volker Bromm ◽  
Naoki Yoshida
Keyword(s):  

Author(s):  
Abraham Loeb ◽  
Steven R. Furlanetto

This chapter examines the intergalactic medium (IGM). Although much of astronomy focuses on the luminous material inside galaxies, the majority of matter today—and the vast majority at z > 6—actually lies outside these structures, in the IGM. This material ultimately provides the fuel for galaxy and cluster formation and—because it is much less affected by the complex physics of galaxies—offers a cleaner view of the underlying physical processes of structure formation and of fundamental cosmology. The chapter thus takes up the study on the properties of the IGM, especially during the era of the first galaxies (when the IGM underwent major changes).


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