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This course on galaxies runs over 14 lectures. The aim is to give you
an overview of galaxy properties and of some of the physical processes
that we think shape galaxies. In contrast to the beauty of stellar
physics, you'll see that galactic physics is often much more murky and
complex - a bit like weather predictions: we (think we) know the
physics, but even so it still is difficult to make accurate
calculations. And often, we don't know the physics very well - or even
at all. On the bright side, galaxies are beautiful. And we can in
principle probe physics on scales which are impossible to reach within
the laboratory and so learn about really fundamental physics - just
recall the recent excitement about the possible non-zero value for the
cosmological constant. Anyway, I hope you'll enjoy the lectures.
As to the organisation of the course, I will basically follow the
structure of Simon Morris, i.e. there will be hand-outs after each
lecture, but more up-to-date versions will appear on the web in
DUO. Look there as well for (most of) the pictures that I show during
the lectures. Suggestions on material included in this course, its
presentation, and lists of errors in the notes, will be most
appreciated.
And for those that are only interested in passing their exams: there
will be two questions on galaxies. The first consist of 5 very short
questions where you're asked to describe very briefly some
concepts that we have discussed. For example, what is the interstellar
medium, and how do we observe it. Given five differences between
football and basketball. The second type of question usually starts from
a derivation that we've done. The end of the question is something you
have not seen, but is very similar to what we have done.
Next: My source of knowledge
Up: Prologue
Previous: Prologue
Tom Theuns
平成19年2月7日