The goal of this lecture is to provide an overview of celestial objects that are sources of high energy radiation (X-ray up to very high energy gamma radiation) in a normal galaxy like our Milky Way. We will discuss the different types of astronomical objects, which are either compact objects formed at the end of a stellar evolution, i.e., white dwarfs, neutron stars, black holes in binary systems, or diffuse emission nebulae formed after a stellar explosion (supernova remnants). To each object types we will present various sub-types and discuss the radiation processes responsible for the observed emission of these objects. A historical overview of observations and theories will be given and the most recent results will be reported, which, as a whole, enable us to improve our knowledge about the composition and the physical processes in the objects.
The lecture will cover the following topics:
The lecture is complementary to the High Energy Astrophysics lecture on Thursday morning. There will be essentially no overlap between the two courses. Taking both courses is therefore encouraged (but by no means mandatory).
The lecture will be given by Prof. A. Santangelo, Dr. M. Sasaki, and Dr. G. Pühlhofer.
Basismodul Astronomie or comparable introductory course in Astronomy and Astrophysics.
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Gerd Pühlhofer
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Last modified 10 Oct 2011 |