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Institut für Astronomie und Astrophysik

Abteilung Astronomie

Sand 1, D-72076 Tübingen, Germany
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Lecture on High Energy Astrophysics WS 2011/12

Contents

Radio Pulsar Sketch
Sketch of the environment of a rotation-powered pulsar. From Chaisson / McMillan, Astronomy Today

The goal of this lecture is to provide an overview of the processes in celestial objects that lead to high energy radiation (X-ray up to very high energy gamma radiation). A main focus of the lecture lies on the radiation mechanisms themselves (e.g. black body radiation, synchrotron radiation). Since the photon energy spectra are intimately related to the state of the matter which releases the radiation (e.g. an accretion disc in a binary system, plasma heated by supernova remnant shocks), we will also introduce some astrophysical processes and environments that produce the highly energetic states of matter. As a matter of fact, those processes are what we want to study when observing high energy spectra of celestial bodies.

The lecture will cover the following topics:

The lecture is not limited to exploring electromagnetic radiation as source of information, other messengers (especially particles) will also eventually be discussed.

The lecture is complementary to the High Energy Sources lecture on Friday 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.

Literature

Prerequisites

Basismodul Astronomie or comparable introductory course in Astronomy and Astrophysics.


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Gerd Pühlhofer | Impressum
Last modified 10 Oct 2011
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