Harvard University
Catalog Number: 4303
Dimitar D. Sasselov
Half course (fall term)
2006, hours (Tu., Th. 2:00-3:30)
in Observatory Classroom (A-101).
Stars are studied as (1) elementary (baryonic) building blocks of the Universe, and (2) main source of the evolution of matter (nucleosynthesis). Planetary systems are studied in terms of the stellar environments for their formation and survival; planets around other stars are compared to Solar system planets.
The NEW Syllabus
(2004) for this course is available as a PostScript file or
PDF.
Course COMPUTER CODES for Stellar Physics.
Final Exam (PS), &
(PDF).
Homework 1,
Homework 2,
Homework 3.
Notes on
Convection (PDF)
Nonradial Oscillations (PPT)
Giant Planet Interiors.II (PPT)
Giant Planet Interiors.III (PPT)
Terrestrial Planets.I (PPT)
Terrestrial Planets.II (PPT)
Exoplanets: Atmospheres (PPT).
Principles of Stellar Evolution and Nucleosynthesis, by D.D. Clayton,
1984, McGraw-Hill (Price: 26.00)
Supernovae and Nucleosynthesis, by D. Arnett, 1996, Princeton (Price:
31.60)
Radiative Processes in Astrophysics, by G.B. Rybicki and A.P. Lightman,
1985, Wiley (Price: 54.95).
Some of the prices quoted above are from the online bookstore
Barnes&Noble where you can get all
or any of these books. They could also
be available from used booksellers online for less, like
abebooks.com.
The first two books contain the basic material.
Questions or Comments? Click here to send me e-mail at dsasselov@cfa.harvard.edu. This page last updated on 09/19/06.