Project information
Circumstellar envelopes of hot stars
- Project Identification
- GA205/04/1267
- Project Period
- 1/2004 - 12/2006
- Investor / Pogramme / Project type
-
Czech Science Foundation
- Standard Projects
- MU Faculty or unit
- Faculty of Science
- Keywords
- astrophysics, stars, hydrodynamics, radiation transfer
- Cooperating Organization
-
Astronomical Institute of the ASCR, v. v. i.
- Responsible person doc. RNDr. Jiří Kubát, CSc.
Circumstellar envelopes of hot stars influence the stellar spectrum and in particular also the stellar evolution. The solution of proposed project will contribute to the understanding of both mentioned relationships. This is why we plan to calculatedetai led models of circumstellar envelopes. We plan to develop more advanced methods on the basis of existing model atmospheres, solution of radiative transfer equation in moving media, and multicomponent stellar wind models. Detailed properties of thesecircu mstellar envelopes will be calculated using mentioned sophisticated models, especially the mass-loss rates. Calculated spectra will be compared with the observed ones both in optical and ultraviolet region. Optical spectra will be acquired usingOndoejov 2m telescope and ultraviolet spectra will be extracted from internet IUE database. More exact wind parameters (mass-loss rates and terminal velocites) will be the output of this part of the project.
Publications
Total number of publications: 30
2005
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Multicomponent stellar winds and chemical peculiarity in A stars
Proceedings of the IAUS224: The A-Star Puzzle, year: 2005
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NLTE wind models of A supergiants
Proceedings of the IAUS224: The A-Star Puzzle, year: 2005
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Radiative transfer in moving media II. Solution of the radiative transfer equation in axial symmetry
Astronomy and Astrophysics, year: 2005, volume: 440
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Spectroscopic and Photometric Observations of SN 2004dj
Information Bulletin on Variable Stars, year: 2005, volume: 2005, edition: 5605
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Stellar winds and the circumstellar environment of massive first stars
From Lithium to Uranium: Elemental Tracers of Early Cosmic Evolution, year: 2005
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Synthetic spectra of A supergiants
Proceedings of the IAUS224: The A-Star Puzzle, year: 2005
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The analyses of the light curves of magnetic CP stars by advanced PCA methods
The A-Star Puzzle, Proceedings IAU Symposium No. 224, 2004, year: 2005
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The dependence of the energy distribution on the abundances of A-star atmosphere models
Proceedings of the IAUS224: The A-Star Puzzle, year: 2005
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The Nature of Light Variations of the He-Strong CP Star HD 37776
Active OB-Stars: Laboratories For Stellar and Circumstellar Physics, year: 2005
2004
-
Challenges to the theories of B stars circumstellar environment
Astronomische Nachrichten, year: 2004, volume: 325, edition: 1