Milky Way Galaxy
B&M = Binney & Merrifield
B&Tr = Binney & Tremaine
MBW = Mo, van den Bosch, White
B&M = Binney & Merrifield
B&Tr = Binney & Tremaine
MBW = Mo, van den Bosch, White
- Gross Properties
- Radial distribution of HI and CO
- Stellar kinematics
- Galaxy models
- Galaxy models
- B&M Sec 10.1 p.609-624
- B&M Sec 9.2.4 p.559-570
- B&M Sec 10.3 p.625-637
- B&M Sec 10.6 p.678-679
- Klypin etal. ApJ, 2002,573.p597
Methods and techniques
- Dynamical time
- Jeans equation and virial theorem
- Two-body relaxation
- Dynamical friction
- B&Tr Sec 2.2.2 p.63-64
- B&Tr Sec 4.8 p.347-364
- B&Tr Sec 7.1 p.554-559
- B&Tr Sec 8.1 p.643-651
Spiral galaxies: Rotation
- Methods, definitions, general trends
- B&M Sec 8.2 p.488-513
Spiral galaxies: photometry
- Trends and Bulge/Disk decomposition
- B&M Sec 4.4.2 p.212-228
Elliptical galaxies
- B&M Sec 4.3.1 p.185-193, 199-210
- B&M Sec. 4.3.3-4 p.194-210
Local Group of Galaxies
- MBW, Sec 2.5.2 p. 71-73
- B&M, Sec. 4.1.4 p.169-172
Luminosity function
- MBW, Sec. 2.4, p.61-67
- B&M, Sec. 4.1.3 p.162-169
Correlation Function
- MBW, Sec. 2.7.1 p.82-83
- MBW, Sec. 6.5 p.283-287
Clusters of Galaxies
- MBW, Sec. 2.5, p.67-71
- Kravtsov, Borgani, 2012. ARA&A 50,353