|
Class meeting date |
Subject |
Reading preparation |
|
|---|---|---|---|
| 1 |
13 January 2005 |
Review of the observed properties of stars I: luminosity; derivation of mass, size and surface temperature from binary systems. Links: Malkov's and Popper's data on binary stars; Terry Herter's binary star simulation; in-class problems and their detailed solution |
Carroll and Ostlie, chapter 7 (pp. 201-221) |
| 2 |
18 January 2005 |
Review of the observed properties of stars II: stellar spectra, spectral classification, and the observed H-R diagram. Links: Stellar spectra from David Silva's Ph.D. thesis, and from Okayama Astrophysical Observatory |
Carroll and Ostlie, chapter 8 (pp. 223-254) |
| 3 |
20 January 2005 |
Stellar atmospheres I: the radiation field and its moments; optical depth. |
Carroll and Ostlie, chapter 9, pp. 255-269 |
| 4 |
25 January 2005 |
Stellar atmospheres II: sources of opacity; the Rosseland mean opacity; the equation of radiative transfer. Links: accurate calculations of the Rosseland mean opacity by the OPAL project |
Carroll and Ostlie, chapter 9, pp. 269-282 |
| 5 |
27 January 2005 |
Stellar atmospheres III: the plane-parallel approximation; gray atmospheres; the Eddington approximation; limb darkening. |
Carroll and Ostlie, chapter 9, pp. 283-292 |
| 6 |
1 February 2005 |
Stellar atmospheres IV: structure of spectral lines; the curve of growth; element abundances. Links: curve-of-growth analysis of Fe I, Fe II, Ti I and Ti II in the Sun's atmosphere: in pdf, or the original Mathcad document |
Carroll and Ostlie, chapter 9, pp. 293-306 |
| 7 |
3 February 2005 |
Stellar atmospheres V: model atmospheres. |
— |
| 8 |
8 February 2005 |
Stellar interiors I: hydrostatic equilibrium; the pressure equation of state. |
Carroll and Ostlie, chapter 10, pp. 315-328 |
| 9 |
10 February 2005 |
Stellar interiors II: nuclear energy sources; fusion; the p-p chains. |
Carroll and Ostlie, chapter 10, pp. 329-344 |
| 10 |
15 February 2005 |
Stellar interiors III: the CNO cycle; energy transport. |
Carroll and Ostlie, chapter 10, pp. 345-355 |
| 11 |
17 February 2005 |
Stellar interiors IV: quick thermodynamics; adiabatic processes and polytropes; convection and mixing-length theory. Links: Magioli's and Cattaneo's movies of computer simulations of stellar convection |
Carroll and Ostlie, chapter 10, pp. 356-365 |
| 12 |
22 February 2005 |
Stellar interiors V: model stellar interiors; the linear stellar model - an approximation that yields an analytical solution with approximately correct behavior; StatStar, a computer solution to the stellar structure equations; the main sequence Links: download StatStar99 from Carroll and Ostlie's website. |
Carroll and Ostlie, chapter 10, pp. 356-365; Stein, pp. 3-38 |
| 13 |
24 February 2005 |
The Sun I: models of the solar interior; the former solar neutrino problem; the solar atmosphere and chromosphere. |
Carroll and Ostlie, chapter 11, pp. 381-405 |
| 14 |
1 March 2005 |
The Sun II: the corona; the solar wind; sunspots, prominences and the solar cycle; polytropes and the Lane-Emden equation. Links: Cool images and movies of sunspot structure from the Dutch Open Telescope and the NASA TRACE satellite |
Carroll and Ostlie, chapter 11, pp. 406-430 |
| 15 |
3 March 2005 |
Post-main-sequence stellar evolution I: evolution on the main sequence; onset of degeneracy. Links: John Lattanzio's stellar-evolution demo |
Carroll and Ostlie, chapter 13, pp. 483-494 |
| 16 |
15 March 2005 |
Post-main-sequence stellar evolution II: full convection, polytropes, and the ascent of the red giant branch; late stellar evolution; planetary nebulae and white-dwarf production, evidence of evolution in stellar clusters.. |
Carroll and Ostlie, chapter 13, pp. 495-516 |
| 17 |
17 March 2005 |
Post-main-sequence evolution III: the fate of massive stars, black hole and neutron-star production, supernovae; explosive nucleosynthesis. |
Carroll and Ostlie, chapter 13, pp. 517-533 |
| 18 |
22 March 2005 |
Stellar pulsation I: Cepheids, RR Lyrae stars, W Virginis stars; the e, k and g mechanisms, the one-zone model.
|
Carroll and Ostlie, chapter 14, pp. 541-556 |
| 19 |
24 March 2005 |
Stellar pulsation II: Models of non-radial
pulsation, p-, f- and g-modes; helio- and asteroseismology. |
Carroll and Ostlie, chapter 14, pp. 557-571 |
| 20 |
29 March 2005 |
Degenerate stars I: white dwarfs; the equation of state of degenerate gases of fermions is polytropic. |
Carroll and Ostlie, chapter 15, pp. 577-591 |
| 21 |
31 March 2005 |
Degenerate stars II: cooling of white dwarfs and the age of the Universe; neutron stars. |
Carroll and Ostlie, chapter 15, pp. 592-607 |
| 22 |
5 April 2005 |
Degenerate stars III: the Chandrasekhar (exact) solution for the structure of a white dwarf. |
— |
| 23 |
7 April 2005 |
Degenerate stars IV: pulsars are rotating neutron stars; pulsars and supernova remnants; pulsar magnetospheres. |
Carroll and Ostlie, chapter 15, pp. 608-626 |
| 24 |
12 April 2005 |
Black holes I: their formation in stellar collapse; elements of the general theory of relativity; the Schwarzschild metric and absolute interval; geodesics, proper time, proper length; gravitational redshift and the Schwarzschild singularity. Links: animations of virtual trips to, and into, black holes: Robert Nemiroff's and Andrew Hamilton's. |
Carroll and Ostlie, chapter 16, pp. 633-648 |
| 25 |
14 April 2005 |
Black holes II: the properties of space and orbits near a Schwarzschild
black hole. |
Carroll and Ostlie, chapter 16, pp. 648-661 |
| 26 |
19 April 2005 |
Black holes III: Rotating black holes and the Kerr metric; black-hole energetics and Hawking radiation; detection of black holes. |
Carroll and Ostlie, chapter 16, pp. 661-676 |
| 27 |
21 April 2005 |
Close binary systems I: Lagrange points and Roche lobes; types of close binary systems; accretion disks. |
Carroll and Ostlie, chapter 17, pp. 683-710 |
| 28 |
26 April 2005 |
Close binary systems II: cataclysmic variables, (white) dwarf novae; neutron stars and black holes in binary systems. |
Carroll and Ostlie, chapter 17, pp. 710-745 |