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Course Criteria
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3.00 Credits
Topics include gravitational equilibrium configurations, virial theorem, polytropes, thermodynamics, convective and radiative transport, stellar atmospheres, nuclear reactions and energy generation, pre-main-sequence contraction, evolution to red giant, white dwarf, and neutron star, and supernova explosions.
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3.00 Credits
Topics include continuum emission mechanisms (synchrotron radiation, inverse compton, and free-free emission), dust emission, photo-ionization and recombination, excitation and transfer of atomic and molecular line broadening, and population inversion and astrophysical masers.
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3.00 Credits
Dynamic and gravitational principles applied to astrophysics. Potential theory, orbital mechanics, virial theorem, Jeans' equations, equilibrium and stability of self-gravitating systems, kinetic theory. Applications to galactic structure and evolution, mergers, dark matter, evolution of star clusters and galactic nuclei and solar system dynamics.
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1.00 - 6.00 Credits
No course description available.
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3.00 Credits
Principles of antennas, receivers, and spectrometers for radio astronomy. Surveys state-of-art systems at centimeter to sub-millimeter wavelengths. Observational techniques and basic system design discussed. There is a laboratory component to course.
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3.00 Credits
Basic numerical methods: linear algebra, interpolation and extrapolation, integration, root finding, extremization and differential equations. Introduction to Monte Carlo techniques used to simulate processes that occur in nature and methods to simulate experiments that measure these processes including random number generators, sampling techniques, and multidimensional simulation. Methods for extracting information from experiments such as experimental measurements and uncertainties, confidence intervals, parameter estimation, likelihood methods, least squares method, hypothesis tests, and goodness of fit tests. Chaotic dynamics and other special topics as time permits.
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3.00 Credits
Describes the gas and dust components of the interstellar medium in ionized regions, atomic clouds, and molecular clouds. Shows how data from optical, infrared, and radio wavelengths can be utilized to determine density, temperature, composition, and dynamics of the various phases of the ISM. Comparison of these results with theoretical models. Includes an overview of the processes that affect the evolution of the ISM including the incorporation of gas and dust into stars, the effect of HII regions and young stellar objects, and the return of matter from evolved stars and supernovae.
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1.00 - 2.00 Credits
Discussion and review of current articles in astronomical literature. May be repeated for credit. Required of graduate students. Credit, 2 each semester.
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1.00 - 2.00 Credits
Discussion and review of current articles in astronomical literature. May be repeated for credit. Required of graduate students. Credit, 2 each semester.
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4.00 Credits
We will explore the issues of sustainability from the perspective of the built environment, our history of construction and expansion, and buildings and how they interact with the natural environment. Students will be exposed to issues of human impacts on natural systems through the built environment and the variety of disciplines that are working to create a more sustainable future. (Gen.Ed. I)
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