
Courses may be offered either in the Fall or Winter Term. Not all courses are offered every year. A list of courses for the upcoming year is circulated at the end of June. A required examination for Ph.D. candidates normally taken at the
beginning of the third term of PhD registration. This six hour, exam tests the student's knowledge of basic astronomy in the fields of the solar system, the Sun and stars, the Milky Way and galaxies, and
cosmology. If necessary, a second attempt is allowed at the end of the third term of study. The exam must be passed in order to continue in the PhD program. Topics include planet formation, orbital and dynamical processes in the
Solar System, isotopes and cosmochemistry, meteorites, asteroids and comets,
planetary interiors and atmospheres as well as other Solar System processes
such as impacts and tides. "Topics include Stellar Dynamics, Galactic structure, Dark Matter,
Interstellar Medium, Spiral Structure, Fluid Mechanics, and
Instabilities." This course will focus on the processes involved in the different stages leading to the formation of stars within our Galaxy. The basic physics and chemistry of the interstellar medium and the current models for low and high mass star formation will be discussed. Special attention will be paid to the observational evidence that support these models or point to their shortcomings. Techniques and methods of infrared astronomy, including imaging,
spectroscopy and interferometry with ground- and space-based
instrumentation. Application to research in star formation, the
interstellar medium, nearby galaxies, and the high-redshift universe. A project-based course consisting of several computationally-intensive
projects suggested by faculty members. Possible project topics include
orbital dynamics, radiative transfer, magnetohydrodynamics, and plasma
astrophysics. The course gives individual faculty members an opportunity
to provide instruction specific to the needs of their students. The astrophysics
behind each project topic will be stressed. This course will include the following topics: the fundamentals of radiative transfer, atomic structure, radiative transitions, radiation from moving charges, bremsstrahlung, synchrotron radiation, and Compton scattering. Topics include relativistic cosmological models; background radiation; cosmological implications of nucleosynthesis; baryogenesis; inflation; structure formation; quasars; intergalactic medium; dark matter and energy. Topics include Maxwell's equations, wave propagation, radiating systems (multipole expansion, Lienard-Wiechart potentials), covariant formulation of electromagnetism. The material covered allows for the discussion and analysis of important examples directly related to important physical phenomena such as Faraday rotation, plasma physics, magnetohydrodynamics, and synchrotron and bremsstralung radiation. This course is intended to provide the student with a thorough introduction to molecular spectroscopy. The emphasis will be on understanding molecules and their spectra by making use of their symmetry (more precisely the symmetry of the Hamiltonian) for problem solving. The necessary tools will be developed to explain the electronic, vibrational, and rotational spectroscopy of simple molecules. We will concentrate on situations involving interactions between gas phase molecules and weak electromagnetic radiation. 3 lecture hours/week. Half course; one term. Half course; one term.
Star Formation in Nearby Galaxies. The physical conditions and process of star
formation in external galaxies, viewed from a multi-wavelength
perspective. The relation of star formation to galaxy
morphology; star formation indicators and the Kennicutt-Schmidt law.
Reading course; half course, one term (offered Summer Term 2008) From its Interior to its Moons. This course aims to examine the physical features of Mars. It will cover the following topics: 1. Mars' core and magnetism based on geochemistry and geodynamics 2. The mantle and crust of Mars based on meteorite petrology and geochemistry 3. The crust of Mars based on volcanology and geomorphology 4. Water on Mars' based on petrology, geomorphology, aqueous geochemistry and salts 5. Weather and climate history on Mars based on remote sensing 6. Mars exploration including findings based on recent missions using remote sensing and geochemical analysis 7. Potential for life on Mars based on geomicrobiology constraints. 8. Mars' moons: Phobos and Deimos. 2 lecture hours/week. Half course; one term. Presentation assignments in the form of one-page abstracts, final exam. 3 lecture hours/week. Half course; one term. 3 lecture hours/week. Half course; one term. 3 lecture hours/week. Half course; one term. This course will introduce students to the processes and products of impact cratering on Earth and throughout the Solar System, including: 1. impact cratering processes; This course will feature weekly lectures, student presentations, hands-on laboratories, and a field trip to the Sudbury impact structure.Astronomy Graduate Courses
9001. Comprehensive Examination
Non-credit requirement.
9601. Solar System and Planetary Astronomy
3 lecture hours/week. Half course; one term. 9602. Galactic Astronomy
3 lecture hours/week. Half course; one term. www.astro.uwo.ca/~basu/teach/ast9602 9603. Star Formation
3 lecture hours/week. Half course; one term. 9604a/b. Galactic and Extragalactic IR Astronomy
3 lecture hours/week. Half course; one term. 9605. Computational Astrophysics
3 lecture hours/week. Half course; one term.9606. Radiative Processes in Astrophysics
3 lecture hours/week. Half course; one term. 9607. Cosmology
3 lecture hours/week. Half course; one term. 9610. Introduction to Modern Astrophysics
This course is an intensive introduction to modern astrophysics. It is expected that all entering Astronomy MSc students will take A9610 in their first term of study (if offered). Topics include: time and coordinate systems; orbits; spectra and radiative processes; the Sun, stars, and stellar evolution; the interstellar medium; the Milky Way and external galaxies; the high-Z universe and cosmology. This course is a pre-requisite for all other astronomy graduate courses (except where noted).
3 lecture hours / week; half course; one term; team taught
9620. Classical Electrodynamics
3 lecture hours/week. Half course; one term.9701. Molecular Symmetry and Spectroscopy
3 lecture hours/week. Half course; one term. 9702. Stellar Atmospheres
9720. Special Topics
9801. Mars
9802. Water in the Solar System
9803. Planetary Image Interpretation (now renumbered Planetary Science 9762)
9601. Planetary Image Interpretation (Combined with GL 9557)
2. the threat;
3. the products of impact cratering;
4. the effects of impact cratering – destructive and beneficial;
5. techniques and research methods;
6. comparative case studies of various impact structures.
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