The First Stars
by Simon C. O. Glover
Publisher: arXiv 2012
Number of pages: 72
The author discusses our current understanding of the physical processes involved in the formation of Population III stars. He shows how we can identify the mass scale of the first dark matter halos to host Population III star formation, and discusses how gas undergoes gravitational collapse within these halos, eventually reaching protostellar densities.
Home page url
Download or read it online for free here:
by Uri Feldman, at al. - ESA Publications Division
Investigations of the heating of the corona and the acceleration of the solar wind are two of the prime scientific goals in studying the solar upper atmosphere with the Solar and Heliospheric Observatory (SOHO) of ESA and NASA.
by George Gamow - Dover Publications
In this fascinating book, a renowned physicist outlines the theories that illuminate the evolution of our world. Gamow employs language that's both scientifically accurate and easy to understand as he traces the development of atomic theory.
by Garrelt Mellema - Leiden University
An introduction to the field of numerical hydrodynamics. It will give you some insight in what is involved in such calculations. Numerical hydrodynamics is used in many parts of astrophysics. The applications we consider in this exercise are stellar.
A supernova is a stellar explosion that briefly outshines an entire galaxy, radiating as much energy as the Sun or any ordinary star is expected to emit over its entire life span, before fading from view over several weeks or months.