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    Figures for Chapter 5 of `Galaxies in the Universe'

    These images are copyrighted and may be used for private purposes only.

  • All Chapter 5 figures as a tar file

  • Figure 5.1: section through a CCD chip (sideways)
  • Figure 5.2: section through a CCD chip (top to bottom)
  • Figure 5.3: NGC 7331 in R-band, CO and H alpha
  • Figure 5.4: NGC 7331 brightness cut showing bulge and disk
  • Figure 5.5: Sombrero galaxy NGC 4594
  • Figure 5.6: Ursa Major group: luminosity and color by type
  • Figure 5.7: edge-on late-type disk galaxies
  • Figure 5.8: Ursa Major group: M(HI)/L by luminosity and surface brightness
  • Figure 5.9: center of M100 showing inner bar
  • Figure 5.10: M95 in UV and optical
  • Figure 5.11: path length for radio interferometer array
  • Figure 5.12: Earth rotation synthesis for radio array
  • Figure 5.13: NGC 7331 in HI
  • Figure 5.14: NGC 7331 HI surface density with radius
  • Figure 5.15: HI mass vs optical and HI diameter for disk galaxies
  • Figure 5.16: NGC 891 in HI, H alpha, radio continuum and optical
  • Figure 5.17: S0 galaxy UGC 7576 with polar ring in HI and optical
  • Figure 5.18: velocity field for rotating disk
  • Figure 5.19: spider diagram for rotating disk
  • Figure 5.20: NGC 7331 rotation curve decomposition
  • Figure 5.21: rotation curves for disk galaxies by type
  • Figure 5.22: NGC 7331 HI global profile
  • Figure 5.23: Ursa Major group Tully-Fisher relation
  • Figure 5.24: UV-optical spectra of disk galaxies
  • Figure 5.25: coarseness, concentration and color by galaxy type
  • Figure 5.26: M100 spiral structure in optical and HI
  • Figure 5.27: NGC 3949, a flocculent spiral
  • Figure 5.28: angles describing spiral pattern
  • Figure 5.29: spiral patterns made from oval orbits
  • Figure 5.30: pattern speeds and resonances in a spiral pattern
  • Figure 5.31: spiral and bar forming in an N-body simulation
  • Figure 5.32: barred galaxy NGC 1300
  • Figure 5.33: simulation of gas flow and orbits in a barred galaxy

    This page last modified: 7 Febuary 2008 (or later if we forgot to change the date)