Physics 612 aSTROPHYSICS (INTERStellar MEDIUM) Course Outline
V. SEMESTER SCHEDULE Class meets MWF at 1:00-1:50 pm in C266 ESC.
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WEEK# |
DATE (2004) | TOPIC |
SUPPL RDG (pp.) |
HW ASSGN DUE |
|
1 |
M Jan 5 | The Interstellar Medium -- an Overview | S 1-17, D&S 1-9 | |
| W Jan 7 | The Two-Level Atom Model | S 70ff, D&S 11ff | ||
| F Jan 9 | ||||
| 2 | M Jan 12 | Spectroscopic Notation | D&S 20ff | |
| W Jan 14 | Application of the Two-Level Atom Model to the 21-cm H Line | |||
| F Jan 16 | Absorption and Emission Features of the IM Spectrum, Molecular Spectra | D&S 24ff | ||
| 3 | M Jan 19 |
M A R T I N L U T H E R K I N G H O L I D A Y |
||
| W Jan 21 | Molecular Spectra | D&S 24ff | ||
| F Jan 23 | Collisional Excitation, the Collisional Strength, Ω(n,n' ) | S 71-87, D&S 41-57 | ||
| 4 | M Jan 26 | Collisional Cooling | ||
| W Jan 28 | Collisional and Radiative Processes in the Three-Level Atom | |||
| F Jan 30 | 1 | |||
| 5 | M Feb 2 | Absorption Lines from the ISM and IGM | S 32-70, D&S 59-100 | |
| W Feb 4 | ||||
| F Feb 6 | Resonance Lines, Zanstra's Method of Finding the UV Flux beyond the Lyman Limit | 2 | ||
| 6 | M Feb 9 | The H 21-cm Line | ||
| W Feb 11 | Galactic Structure Inferred from 21-cm Observations | S 42-50, D&S 75-81 | ||
| F Feb 13 | The Bowen Fluorescence Mechanism | D&S 82-85 | ||
| 7 | M Feb 16 |
P R E S I D E N T S ' D A Y H O L I D A Y |
||
| T Feb 17 | (Monday Class Instruction) The Bowen Fluorescence Mechanism | |||
| W Feb 18 | Astronomical Masers | S 44-46, D&S 88-99 | ||
| F Feb 20 | Line Recombination Spectra |
S 105-111, D&S 105-108, 138-142 |
||
| 8 | M Feb 23 | |||
| W Feb 25 | Two-Photon Emission | D&S 135-138, 398-400 | ||
| F Feb 27 | Continuum Recombination Spectra | S 105-107, D&S 132-133 | ||
| 9 | M Mar 1 | Free-Free Spectra | S 57-68, D&S 125-132, 243 | |
| W Mar 3 | Curve-of-Growth Applications to Interstellar Cloud Spectra | S 46-57, D&S 60-67 | 3 | |
| F Mar 5 | ||||
| 10 | M Mar 8 | Interstellar Dust (Evidences for, Formation) | S 205-213, D&S 289-295 | |
| W Mar 10 | Midterm Test (Conceptual, Open Book) | See above (Jan 5 - Mar 5) | ||
| F Mar 12 | Interstellar Dust (Optical Properties) | S 149-170, D&S 296-324 | ||
| 11 | M Mar 15 | The Standard Reddening Law | ||
| W Mar 17 | Optical Efficiencies, Polarization | |||
| F Mar 19 | Polarization | S 65-68 | ||
| 12 | M Mar 22 | Faraday Rotation, Rotation Measure and Dispersion Measure | S 61-62, 65-68; D&S 168-169 | |
| W Mar 24 | The Galactic Magnetic Field | S 10-11 | 4 | |
| F Mar 26 | ||||
| 13 | M Mar 29 | Strömgren Spheres, H II Regions | S 103-111, D&S 220-225 | 5 |
| W Mar 31 | ||||
| F Apr 2 | Fossil Strömgren Spheres, Shock Fronts |
S 218-222 |
||
| 14 | M Apr 5 | Ionization Fronts | S 247-250, D&S 225-230 | 6 |
| W Apr 7 | ||||
| F Apr 9 | Helium Ionization (He II) | S 111, D&S 138-140 | ||
| 15 | M Apr 12 | Helium Ionization (He II and He III) | ||
| W Apr 14 | R E A D I N G D A Y S | |||
| Q Apr 15 | ||||
| 16 | T Apr 20 |
F I N A L E X A M I N A T I O N (7 pm) |
Final |