Project information
Physics of Sun, stars, and stellar systems
- Project Identification
- GD205/08/H005
- Project Period
- 1/2008 - 12/2011
- Investor / Pogramme / Project type
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Czech Science Foundation
- Doctor grants
- MU Faculty or unit
- Faculty of Science
- Keywords
- x
- Cooperating Organization
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Astronomical Institute of the ASCR, v. v. i.
- Responsible person doc. RNDr. Jiří Kubát, CSc.
Contemporary astrophysics is one of the most dynamic scientific branches thanks to continuous development of observing techniques and of its the theoretical base, which exploits results of related sciences, especially physics. Demands on young scholars, who have to manage both observing techniques and theoretical astrophysics, are very high. They can be fulfilled only by common effort of all institutes interested both in research and education. Proposed project aims at a contribution to student education by their involvement in the research of radiative processes and magnetohydrodynamics of astrophysical plasma, which exists in Sun, stars, stellar systems and their surroundings. Plasma behaviour and properties then determine the character of stellar and stellar systems inner structure and their evolution. The project consists also of targeted astrophysical observations, which will bring information allowing tests of the findings. Naturally, also observation of Sun, stars, and stellar systems
Publications
Total number of publications: 46
2009
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The circumbinary dusty disk around the hydrogen-deficient binary star upsilon Sagittarii
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The nature of the light variability of the silicon star HR 7224
Astronomy and Astrophysics, year: 2009, volume: 37, edition: 499
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Transient Jets in the Symbiotic Prototype Z Andromedae
Astrophysical Journal, year: 2009, volume: 690, edition: 2
2008
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Photometry of extrasolar planets
Proceedings of the 40th Conference on Variable Stars Research, year: 2008
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Rotational periods of magnetic chemically peculiar stars
XVI. Ulusal astronomi kongresi, V. Ulusal ögrenci astronomi kongresi, year: 2008
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The nature of the light variations of chemically peculiar stars
Ulusal astronomi kongresi, year: 2008