by P.K. Townsend
Publisher: arXiv 1997
Number of pages: 145
These notes were written to accompany a course taught in Part III of the Cambridge University Mathematical Tripos. From the table of contents: Gravitational Collapse; Schwarzschild Black Hole; Charged Black Holes; Rotating Black Holes; Energy and Angular Momentum; Black Hole Mechanics; Hawking Radiation.
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by James N. Pierce - Minnesota State University
This book provides an introduction to the details of the structure, operation, and evolution of stars. It will be most useful to undergraduates in upper-level astronomy courses and graduate students taking Stellar Interiors or Stellar Atmospheres.
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 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.