. "Astrophysics"@en . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . "Astrophysics I"@en . . "5" . "Introduction, basic definitions, stellar parameters: Astronomy as an observational science,\nastrophysics. Celestial sphere, coordinate systems used in astronomy. Stellar parallax,\ncosmic distance scale, distance ladder. Blackbody radiation. Stellar spectra, flux, effective\ntemperature. Spectral classification. Magnitude scale, bolometric magnitude, luminosity,\ncolour index. Stellar parameters. Determination of stellar masses and radii. Hertzsprung-\nRussell diagram. Tools of astrophysics: Electromagnetic spectrum, observing windows.\nGround-based and space observatories. Telescopes. Detectors. Infrared, ultraviolet, X-ray\nand gamma astronomy. Observing techniques: imaging. Observing techniques: photometry.\nObserving techniques: spectroscopy. Observing techniques: optical and radio interferometry.\nObserving techniques: astrometry. Observing techniques: polarimetry. Stellar atmospheres:\nDescription of radiation field. Interaction of light and matter, stellar opacity. Radiative and\nconvective transfer. Transfer equation and its formal solution. Equations of hydrostatic and\nradiation equilibrium. Gray atmosphere, diffusion approximation, LTE approximation. Models\nof stellar atmospheres. Spectral lines and their profiles, formation of spectral lines.\nAtmospheric abundances of stars. Ages of stars. Stellar structure and evolution: Interstellar\nmatter (IM), dust and gas, absorption by IM. Formation of stars, virial theorem, the Jeans\nmass. Pre-main sequence evolution. Stellar interiors, hydrostatic equilibrium. Basic\nequations. Sources of stellar energy, opacity, equation of state, transport of energy. Models\nof stellar interiors. Degeneracy of matter. Main-sequence evolution. Post-main-sequence\nevolution. Testing the theory of stellar evolution (stellar clusters, stellar pulsations). Stellar\nvariability and its origin. The Sun: Solar interior. Solar atmosphere. Activity of the Sun, solar\ncycle. Solar pulsations. Solar neutrino problem." . . "Presential"@en . "TRUE" . . "Master in Astrophysics"@en . . "https://international.uni.wroc.pl/en/admission-full-degree-studies/programmes-english/astrophysics" . "no data" . "Presential"@en . "The program comprises only a few mandatory courses that acquaint you with general foundations of astrophysics, necessary computer simulation tools and data analysis methods, as well as selected observational techniques. This is supplemented by a wide range of elective courses enabling you to deepen your knowledge and skills according to your scientific interest. You can follow astronomy- or physics-oriented study track that will prepare you for the Master project held in the Astronomical Institute or the Institute of Theoretical Physics, respectively.\nIn the course of becoming an educated astrophysicist, you will gain expertize in mathematical modeling, computer simulations and advanced data analysis. You will also develop universal research competencies, including analytical and critical thinking, rigorous evidence-based reasoning, creativity and complex problem solving, active learning, as well as communication and teamwork skills."@en . . . . "2"@en . "TRUE" . . "Master"@en . "no data" . "1000.00" . "Euro"@en . "2150" . "no data" . "The modern job market awaits people with your competencies! Upon graduation, you will be capable of working in academy, R&D institutes and centers of education, as well as in various knowledge-based economy branches, including ICT, high-tech industry or financial institutions. However, you will be particularly well-prepared to undertake PhD studies and continue scientific career."@en . "no data" . "TRUE" . "Upstream"@en . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .