next up previous contents
Next: List of Tables Up: thesis Previous: Contents   Contents


List of Figures

  1. Number of Cepheids vs Age for MC Clusters
  2. NGC 330 finding chart
  3. NGC 330 field CMD
  4. NGC 330 cluster CMD
  5. NGC 300 Cepheid variable light curves
  6. NGC 330 LPV light curves
  7. NGC 330 Semi-regular and irregular variable light curves
  8. Light curves for the eclipsing and binary variables
  9. Evolutionary tracks for masses M = 2.5, 3.5 and 5M$\scriptstyle \odot$, Y = 0.25 and Z = 0.004
  10. The SMC PL relation and PLC relation, with no overshoot
  11. The SMC PL and PLC relation with a large amount of overshoot
  12. The Hα emission profiles of the binaries 66V and 77V
  13. NGC 1850 finding chart
  14. NGC 1850 field CMD
  15. NGC 1850 cluster CMD
  16. NGC 1850 Cepheid variable light curves
  17. NGC 1850 core finding chart
  18. NGC 1850 LPV light curves
  19. NGC 1850 Semi-regular variable light curves
  20. NGC 1850 RR-Lyrae variable light curves
  21. NGC 1850 dereddened Colour-Magnitude diagram
  22. Comparison of evolution mass and pulsation mass for NGC 1850 Cepheids
  23. Bump Cepheid models compared to HV905
  24. Light and colour curves for HV905
  25. The observed PLC compared with theory
  26. The K-logP relation for NGC 1850 LPVs
  27. The NGC 2058-65 field finding chart
  28. Finding charts for NGC 2059, 2058 and 2065
  29. The Colour-Magnitude diagram for the NGC 2058-65 field
  30. The Colour-Magnitude diagram for NGC 2058
  31. The Colour-Magnitude diagram for NGC 2065
  32. Light curves of the Cepheid variables
  33. The light curves of the Long-Period Variables
  34. Light curves for the unusual and eclipsing variables
  35. The NGC 2058-65 field with overlaid isochrones
  36. The reddening-independent P-L diagram for NGC 1850, NGC 1866 and NGC 2058-65
  37. The LMC Period-Luminosity diagram
  38. The NGC 2058-65 Period-Luminosity-Colour diagram
  39. Comparison of evolution and pulsation masses
  40. The NGC 2058-65 LPV K-logP diagram
  41. The LPVs in the (K0,logP) plane
  42. The I band amplitude distribution for the two LPV sequences
  43. The NGC 1850 CMD with the LPVs and theoretical AGB tracks marked
  44. The observations of LPVs compared with theoretical models in the (K,logP) plane
  45. As for Figure 5.4 except that the first-overtone period has been forced to fit the observed Mira (K,logP) relation.
  46. Period-Luminosity diagram for 0.8, 1.0 and 1.5M$\scriptstyle \odot$ model AGB stars

Kim Sebo 2008-06-20