. "Galactic astronomy"@en . . "5" . "General structure of the Galaxy. Interchange of matter between stars and ISM. Forms of\nISM: gas and dust, extinction, reddening. Stellar clusters: globular and open, moving cluster.\nMilky Way in near and far infrared. Velocity of the Sun with respect to neighbouring stars:\napex, centroid. LSR and peculiar velocities. Determination of Solar LSR velocity in respect to\nthe Galaxy centre. Determination of the peculiar velocity of the Sun. Simple model of the\nGalaxy rotation: velocity vector of a star in respect to the Sun. Oort's approach to the Galaxy\nrotation. Oort's constants. Differential rotation of the Galaxy: geometric interpretation.\nGalactic rotation curve from radio observations of HI clouds. Determination of the Sun –\ngalactic center distance. Estimation of the Galaxy mass from Oort's constants. Models of\nmass distribution in the Galaxy. Surface brightness of galaxies. Visual versus dynamical mass\nof the Galaxy. Dark matter. Distribution of stellar velocities: fast and slow stars, orbits.\nDistribution of components of peculiar velocities for slow stars: ellipsoid and dispersion.\nRelationship between velocity dispersion, spectral type and metallicity. Asymetric distribution\nof the rotational component of the peculiar velicities. Scattering of the stellar orbits leading\nto the increase of the peculiar velocity dispersion. Disc and halo kinematics. Star counts\nmethodology. Relation between star-counts and their space distribution. Kapteyn's universe.\nLF, ILF and SFR functions. LF for galactic disc and for stars in GC. Height scale and its\ndependence on spectral type. Discovery of spiral arms in the Galaxy. Stability of spiral arms\nand density waves. Mechanism of star formation in spiral arms. Discovery of galactic bar.\nStellar populations of the Galaxy. Thin and thick discs. Gas and dust distribution in the\nGalaxy. ELS model of the Galaxy orogin: free infall and energy dissipation. SZ model of the\nGalaxy formation: acrection. Chemical evolution of the Galaxy. Age and spatial distribution\nof globular clusters. Origin of the thick disc. Centre of the Galaxy with a black hole." . . "Presential"@en . "FALSE" . . "Other Astronomy Kas"@en . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . "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 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .