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 First Galaxies in the Universe 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. Provides a comprehensive introduction to this exciting frontier in astrophysics Begins from first principles Covers advanced topics such as the first stars and 21-cm cosmology Prepares students for research using the next generation of large telescopes Discusses many open questions to be explored in the coming decade
This book offers a succinct and accessible primer at a time when breathtaking technological advances promise a wealth of new observational data on the first stars and galaxies.
Together, they will revolutionize the study of the most distant objects in the Universe. This volume is aimed at beginning graduate students but can also serve as a reference work for active researchers in the field.
For relevant physics, an undergraduate text using SI units is M. S. Longair, High Energy Astrophysics, ... Volume 1, Particles, Photons and their Detection; 1994, Volume 2, Stars, the Galaxy and the Interstellar Medium.
This book takes the reader on an exploration of the structure and evolution of our universe.
Galaxies are vast ensembles of stars, gas and dust, embedded in dark matter halos. They are the basic building blocks of the Universe, gathered in groups, clusters and super-clusters. They exist in many forms, either as spheroids or disks.
This is left as key science for future telecopes like the James Webb Space Telescope.
A comprehensive examination of nearly fourteen billion years of galaxy formation and evolution, from primordial gas to present-day galaxies.
Fundamentals of Galaxy Dynamics, Formation and Evolution is written for advanced undergraduates and beginning postgraduate students, providing a useful tool to get up to speed in a starting research career.
Consequently, the flux in forbidden lines is not directly related to the UV luminosity produced by massive young stars. Despite of this, it is found that the [OII] ... (d) Far-Infrared Continuum Typically the ISM associated with a ...
McDonald, P., Seljak, U., Burles, S., Schlegel, D.J., Weinberg, D.H., Cen, R., D., S., Schaye,J., Schneider,D.P.,Bahcall,N.A.,Briggs,J.,Brinkmann,J.,Brunner,R.J., ... Mitchell, J.L., Keeton, C.R., Frieman, J.A., and Sheth, R.K. (2005).