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Content archived on 2024-05-21

Accretion disks, Jets, and High Energy Phenomena in Astrophysics

Objective

The aim of the school is to bring an up-to-date formation in the theory and the observational facts concerning accretion and its related phenomena, jet production and high-energy emission in astrophysical objects. We aim also in providing practical training for the use of new generation instruments suited for the study of such phenomena. Accretion process is thought to play a major role in many places in the Universe: the star formation must take place through the collapse of molecular clouds towards a core, the final stage being the formation accretion disk feeding the young star; Active Galactic Nuclei are very probably due to accretion onto a super massive black hole in the centre of galaxies; cataclysmic variables and X -ray binaries are also the result of accretion of a companion star onto a stellar mass compact object, either a white dwarf, a neutron star or a stellar black hole. Gamma-ray bursts are also believed to be produced by the release of enormous amount of energy during a violent accretion process, being probably the final stage leading to a black hole through either the coalescence of two compact objects or the final collapse of a very massive star.

The formation of jets seems to be ubiquitous in all these phenomena, and are associated in some cases with very high energy emission. Despite very different physical conditions, it seems that the basic picture based on magneto-hydrodynamics could account for all these phenomena, but the details are still the subject of intensive research. In 2002 or in the very next years, new instruments with unprecedented sensitivities, energy and angular resolution will be ready to provide new information about all these objects in various wavelength domains: radio (ALMA) and optical (VLTI) interferometers, X-ray (CHANDRA, XMM, INTEGRAL) and gamma-ray (GLAST, AMS) satellites, very high energy ground detectors (HESS, AUGER, ANTARES)... Many of them have been designed by a European collaboration, or an international one with a strong involvement of EU. The school will bring the opportunity of giving the most recent results obtained or expected with these instruments. It will also include practical training for using the most up-to-date techniques and contribute thus to their best use by young researchers.

Fields of science (EuroSciVoc)

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Topic(s)

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Call for proposal

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Funding Scheme

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ACM - Preparatory, accompanying and support measures

Coordinator

Type of Event: Euro Summer School
EU contribution
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Address
This event takes place in Les Houches

France

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Total cost

The total costs incurred by this organisation to participate in the project, including direct and indirect costs. This amount is a subset of the overall project budget.

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