Graduate Program | Courses
Fall 2009
Astronomy 520: Computational Methods for Astrophysics and Geophysics
| Instructor |
Paolo Coppi |
| Location/Time |
Gibbs 263, Gibbs 502, T 1:15 - 2:30, Th 12:50 - 2:00 |
| Prerequisites |
ASTR 320b, MATH 120a or b, 222a or b or 225a or b, and 246a or b. |
| Description |
The analytic and numerical/computational tools necessary for effective research in astronomy, geophysics, and related disciplines. Topics include numerical solutions to differential equations, spectral methods, and Monte Carlo simulations. Applications are made to common astrophysical and geophysical problems including fluids and N-body simulations. |
Astronomy 555: Observational Techniques
| Instructor |
Robert Zinn |
| Location/Time |
Gibbs 263, T Th 10:30-11:20 1HTBA |
| Course Web Page |
View Course Site |
| Description |
The design and use of optical telescopes, cameras, spectrographs, and detectors to make astronomical observations. The reduction and analysis of photometric and spectroscopic observations. |
Astronomy 570: High Energy Astrophysics
| Instructor |
Eilat Glikman |
| Location/Time |
Gibbs 263, M W 10:30-11:45 1HTBA |
| Description |
A survey of current topics in high-energy astrophysics, including accreting black hole and neutron star systems in our galaxy, pulsars, active galactic nuclei and relativistic jets, gamma-ray bursts, and ultra-high-energy cosmic rays. The basic physical processes underlying the observed high-energy phenomena are also covered. |
Astronomy 580: Research
| Instructor |
|
| Description |
By arrangement with faculty. |
Astronomy 600: Cosmology
| Instructor |
Priyamvada Natarajan |
| Location/Time |
Gibbs 263, T Th 9:00-10:15 |
| Description |
A comprehensive introduction to cosmology at the graduate level. The standard paradigm for the formation, growth, and evolution of structure in the Universe is covered in detail. The course does not assume prior knowledge of general relativity. |
Astronomy 666: Statistical Thermodynamics for Astrophysics and Geophysics
| Instructor |
|
| Location/Time |
KGL 119, T Th 2:30 - 3:45 |
| Description |
Classical thermodynamics is derived from statistical thermodynamics. We then develop kinetics, transport theory, and reciprocity from the linear thermodynamics of irreversible processes. Emphasis is placed on phase transitions, including novel states of matter, nucleation theory, and the thermodynamics of atmospheres. We explore phenomena that are of direct relevance to problems in astrophysical settings, atmospheres, oceans, and the Earth's interior. No quantum mechanics is necessary as a prerequisite. |
Astronomy 710: Professional Seminar
| Instructor |
Richard B. Larson |
| Location/Time |
Gibbs 263, F 1:30 - 3:00 |
| Description |
A weekly seminar covering science and professional issues Astronomy. |
Image Credits: (header) Carolin Cardamone
