Oxford
Physics:
Third-Year Astrophysics (B3)

Stellar Structure and
Evolution

(Dr Ph. Podsiadlowski)
Lecture Schedule and
Individual Lecture Notes: Michaelmas 2006
- Lecture
1: (pdf files: B/W, colour)

Introduction, observable properties of
stars, magnitudes,
stellar classification

- Lecture 2: (pdf
files: B/W, colour)

Stellar properties, H-R (CM) diagrams,
star clusters, stellar
populations, brown dwarfs, planets

- Lectures 3/4
: (pdf files: B/W, colour)

Equations of stellar structure:
hydrostatic equilibrium,
virial
theorem, stellar timescales, energy transport by radiation and
convection

- Lecture 5: (pdf
files: B/W, colour)

The mathematical problem, equations of state, opacities

- Lecture 6: (pdf
files: B/W, colour)

Nuclear reactions: nuclear binding
energy,
the Coulomb barrier, non-resonant reaction rates, hydrogen burning (pp
chains,
CN cycle), helium burning

(pdf files: B/W, colour)

The Sun: helioseismology, the solar
neutrino problem
- Lectures
7/8: (pdf
files: B/W, colour)

The structure of main-sequence stars, ages in open clusters, star formation,
The evolution of low-mass stars: the
red-giant
phase, the helium flash, the horizontal branch, the asymptotic giant
branch,
planetary nebulae, white dwarfs, the Chandrasekhar mass

- Lecture 9: (pdf
files: B/W, colour)

The evolution of massive stars, supernova types: core collapse and
thermonuclear
explosions, supernova classification, SN 1987A, neutron stars, black
holes, gamma-ray bursts
(pdf files:
B/W, colour)

Binary stars: classification, the mass
function,
the Roche potential, mass transfer, the Algol paradox, binaries
with compact components
Homepage