Harvard University
Catalog Number: 4303
Dimitar D. Sasselov
Half course (fall term)
2008, hours (Mon, Wed. 11:15-12:40)
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
(2008) for this course is available as a PostScript file or
PDF.
Course COMPUTER CODES for Stellar Physics.
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).
You could also find useful the following books, if you have them:
Planetary Sciences, by I. dePater & J. Lissauer, 2001, Cambridge UP
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).
Questions or Comments? Click here to send me e-mail at dsasselov@cfa.harvard.edu. This page last updated on 09/12/08.