Harvard University
Catalog Number: 2128
Dimitar D. Sasselov
Half course (fall term)
2002, hours (Tu., Th. 10:10-11:30)
in Observatory Classroom (A-101).
Stellar physics is studied from the two basic precepts -
of the elementary (baryonic) building blocks in the Universe and the evolution
of matter (nucleosynthesis). The theory of stellar interiors and atmospheres
is developed from general grounds and applied as fit to the
variety of stellar objects and their environments. The observational methods
(spectroscopy, dynamics, and seismology) are also discussed briefly. The
goal is to provide the student with basic tools for further research and
with an overall picture of the evolution of matter in the Universe.
Exploring the physics and parameter space with the provided
computer codes on the Web page is strongly encouraged.
The NEW Syllabus
(2002) for this course is available as a PostScript file.
Problem Set 1 (SOLUTIONS [PDF]);
Problem Set 2;
Problem Set 3 (SOLUTIONS [PDF]);
Problem Set 4
[
PDF];
Problem Set 5
[
PDF].
FINAL Exam
[
PDF] (due January 21, 2003, 12 noon, in DS or TF's offices or m-boxes).
Questions or Comments? Click here to send me e-mail at dsasselov@cfa.harvard.edu. This page last updated on 09/20/02.