Lecture slides (part 1) - Vanderbilt Astronomy Group
Lecture slides (part 1) - Vanderbilt Astronomy Group Lecture slides (part 1) - Vanderbilt Astronomy Group
from astro.phy.vanderbilt.edu
More from this publisher
27.10.2014
Views
A galaxy cluster: Dark matter 85% of mass
A galaxy cluster: Hot X-ray gas 12% of mass
- Page 215 and 216: Measured galaxy properties What can
- Page 217 and 218: Measured galaxy properties What can
- Page 219 and 220: Galaxy light profiles Disk galaxies
- Page 221 and 222: Galaxy light profiles More general:
- Page 223 and 224: Galaxy light profiles
- Page 225 and 226: Galaxy morphology Spiral S0/lenticu
- Page 227 and 228: Galaxy morphology Types • Spiral
- Page 229 and 230: Galaxy morphology 1D fitting de Sou
- Page 231 and 232: Galaxy morphology • 150,000 peopl
- Page 233 and 234: Galaxy environments
- Page 235 and 236: Galaxy environments • Galaxy dens
- Page 237 and 238: Galaxy environments Small group (N=
- Page 239 and 240: Galaxy environments In a void • G
- Page 241 and 242: Morphology-density relations Bamfor
- Page 243 and 244: Correlations of galaxy properties w
- Page 245 and 246: Galaxy groups and clusters What def
- Page 247 and 248: Galaxy groups and clusters Geometri
- Page 249 and 250: Galaxy groups and clusters Berlind
- Page 251 and 252: Galaxy groups and clusters Berlind
- Page 253 and 254: Galaxy groups and clusters 2D Photo
- Page 255 and 256: Galaxy groups and clusters g-r g-r
- Page 257 and 258: Galaxy groups and clusters X-ray cl
- Page 259 and 260: Galaxy groups and clusters X-ray cl
- Page 261 and 262: Galaxy groups and clusters SZ clust
- Page 263 and 264: Galaxy rotation curves Instead, it
- Page 265: How does MOND work? F = GMm r 2 = m
- Page 269 and 270: Galaxies
- Page 271 and 272: Dark matter
- Page 273 and 274: Gravitational lensing
- Page 275 and 276: Optical image
- Page 277 and 278: Modelling
- Page 279 and 280: What happens in a cluster collision
- Page 281 and 282: What happens in a cluster collision
- Page 283 and 284: X-ray image
- Page 285 and 286: Lensing map
A galaxy cluster: Hot X-ray gas<br />
12% of mass
Change language