Multiwavelenght observations and analysis of the selected active stars
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Abstract (EN)
Magnetic activity drives high-energy processes in the atmosphere?s of stars. Powerful reconnection events (stellar flares) are regularly observed. Such processes give rise to observable effects across the electromagnetic spectrum, from the microwave region to hard X-rays. Even so, full details of the electron dynamics associated with these emissions remain incompletely observed and not properly understood.In this thesis, we propose to multiwavelenght approach to analysis of four active stars, such as YY Gem, AB Dor, CC Eri and HD 191588 that we have access to relevant data.
Author
Naci Erkan
How to Cite
Naci Erkan (Doctorate thesis). Multiwavelenght observations and analysis of the selected active stars, 2012, Çanakkale Onsekiz Mart University.
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